hypergiant, together with the red supergiants Mu Cephei, MY Cephei, VV Cephei, V381 Cephei, and V354 Cephei are among the largest stars known. In addition...

Mu Cephei is a red supergiant or hypergiant star in the northern constellation Cepheus. It is officially named the Garnet Star; Mu Cephei is its Bayer...

VV Cephei, also known as HD 208816, is an eclipsing binary star system located in the constellation Cepheus. It is both a B[e] star and shell star. As...

Gamma Cephei is a binary star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from γ Cephei, and abbreviated...

asterism consisting of α Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Xi Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese...

Cephei is a quadruple star system in the northern constellation of Cepheus, the King. Its name is a Bayer designation that is Latinized from δ Cephei...

V354 Cephei (abbreviated to V354 Cep) is a red supergiant star located within the northern constellation of Cepheus. It is an irregular variable located...

S Cephei (S Cep), also designated as HD 206362, is a carbon star and Mira-type variable in the constellation Cepheus. Based on the measurement of its annual...

W Cephei is a spectroscopic binary and variable star located in the constellation Cepheus. It is thought to be a member of the Cep OB1 stellar association...

Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations...

Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements can be inconsistent...

U Cephei is an eclipsing binary star discovered in 1880. It consists of a blue-white main sequence star of spectral type B7/8V that is eclipsed every two...

Beta Cephei is a triple star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from β Cephei, and abbreviated...

Gamma Cephei Ab (abbreviated γ Cephei Ab, γ Cep Ab), formally named Tadmor /ˈtædmɔːr/, is an exoplanet approximately 45 light-years away in the constellation...

designation Rho Cephei (ρ Cephei / ρ Cep) is shared by two stars in the constellation Cepheus: ρ1 Cephei ρ2 Cephei, often called just ρ Cephei This set index...

Epsilon Cephei is a star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ε Cephei, and abbreviated Epsilon...

Labelled Omega Cephei (ω Cep/ω Cephei) by Bode in his Uranographia Designated by Burrett in his atlas Labelled Tau Cephei (τ Cep/τ Cephei) by Bode in his...

asterism consisting of Xi Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Alpha Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese...

SS Cephei is a semiregular variable star in the constellation Cepheus. It is of spectral type M5III, and has an estimated temperature of about 3,700 K...

Zeta Cephei is a red supergiant star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ζ Cephei, and abbreviated...

RW Cephei is a K-type hypergiant and a semirregular variable star in the constellation Cepheus, at the edge of the Sharpless 132 H II region and close...

consisting of η Cephei, 4 Cephei, HD 194298, θ Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei. Consequently, the Chinese name for η Cephei itself...

ST Cephei (ST Cep), also known as BD+56°2793, is a red supergiant and a variable star located in the constellation Cepheus. It has a variable apparent...

MY Cephei (abbreviated to MY Cep), also known as IRC +60375, is a red supergiant or hypergiant located in the open cluster NGC 7419 in the constellation...

consisting of 4 Cephei, HD 194298, η Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei. Consequently, the Chinese name for θ Cephei itself is 天鈎三...

LZ Cephei, also known by its Flamsteed designation 14 Cephei, is a star about 3,600 light years from the Earth, in the constellation Cepheus. Its apparent...

Omicron Cephei is a binary star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ο Cephei, and abbreviated...

V381 Cephei (HR 8164) is a triple star system in the northern constellation of Cepheus. Its apparent magnitude is slightly variable between 5.5 and 5.7...

Pi Cephei is a trinary star system located in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from π Cephei, and...

Rho2 Cephei is a solitary star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ2 Cephei, or simply ρ...

Nu Cephei is a blue-hued variable star in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from ν Cephei, and abbreviated...

Iota Cephei is a star in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from ι Cephei, and abbreviated Iota Cep...

AR Cephei (AR Cep) is a variable star in the constellation Cepheus. It is classified as a semiregular star with a spectral type of M4III. Aernout de Sitter...

9 Cephei (9 Cep), also known as V337 Cephei, is a variable star in the constellation Cepheus. It is visible to the naked eye. In 1967, Graham Hill announced...

V Cephei is a white main sequence star in the constellation Cepheus. It only varies slightly by 0.03 of a magnitude. It was suspected of being variable...

hypergiant that may also challenge the Humphreys–Davidson limit UY Scuti MY Cephei Mistakenly referred to as RSGC1-01. Calculated, using the Stefan-Boltzmann...

Tauri star PV Cephei. It is known for changing its shape dramatically on a timescale of months to years, as the brightness of PV Cephei changes. The nebula...

Lambda Cephei is a blue supergiant star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from λ Cephei, and is...

V355 Cephei is a red supergiant located in the constellation of Cepheus. It has a radius between 770±154 and 790 solar radii, making it one of the largest...

DH Cephei is a variable binary star system in the northern circumpolar constellation of Cepheus, positioned about two degrees to the east of the star system...

Rho1 Cephei is a double star located in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ1 Cephei, and abbreviated...

Krüger 60 (DO Cephei) is a binary star system located 13.1 light-years (4.0 parsecs) from Earth, being one of the nearest stars. It is made up of a pair...

T Cephei is a Mira variable star in the constellation Cepheus. Located approximately 600 light-years (180 parsecs) distant, it varies between magnitudes...

helium is doubly ionized. The term Cepheid originates from the star Delta Cephei in the constellation Cepheus, which was one of the early discoveries. On...

Cephei ("Errai") by 3000 AD, with Errai reaching its closest alignment with the northern celestial pole around 4200 AD. Iota Cephei and Beta Cephei will...

cooler stars and even detected in giant hot stars such as Betelgeuse, Mu Cephei, Antares and Arcturus. Circumstellar disks: including those of more than...

Cephei is a binary star system in the northern circumpolar constellation of Cepheus. Its name is a Bayer designation that is Latinized from κ Cephei,...

located near the Mira-type variable star T Cephei, and near the bright magnitude +3.23 variable star Beta Cephei (Alfirk). The designation NGC 7023 refers...

V419 Cephei (BD+59°2342 or HIP 104719) is an irregular variable star in the constellation of Cepheus with an apparent magnitude that varies between 6.54...

19 Cephei is a supergiant star in the northern circumpolar constellation of Cepheus. It has a spectral class of O9 and is a member of Cep OB2, an OB association...

system located in the constellation of Scutum. It is classified as a VV Cephei-type system, which typically consists of a cool red supergiant and a hot...

rise to maximum light followed by a slower fall to minimum (e.g. Delta Cephei). This is due to the phase difference between the radius and temperature...

Tsuji, T. (2000). "Water on the early M supergiant stars α Orionis and μ Cephei". The Astrophysical Journal. 538 (2): 801–07. Bibcode:2000ApJ...538..801T...

VW Cephei (VW Cep) is a triple star in the constellation Cepheus, located roughly at 90.6 light years from the Sun. The two inner components form an eclipsing...

constellation Hercules, 139 parsecs (450 light-years) away. The brightest is a β Cephei variable, a pulsating star. Iota Herculis (Latinized from ι Herculis, abbreviated...

four largest galactic red supergiants per a survey, including Mu Cephei and V354 Cephei, along with later the extragalactic star, WOH G64 A, which used...

WZ Cephei is an eclipsing binary star of W Ursae Majoris-type in the constellation of Cepheus, located 976 light years away from the Sun. The stars orbit...

understood to be high-order gravity modes excited by the kappa mechanism. Beta Cephei variables are slightly hotter (and thus more massive), also have modes excited...

PV Cephei is a variable star of Orion type located in the constellation of Cepheus at a distance of about 1,100 light-years from Earth. In visible light...

11 Cephei is a single star in the northern constellation of Cepheus, located 179 light years away from the Sun. It is visible to the naked eye as a faint...

In astronomy, a semiregular variable star, a type of variable star, is a giant or supergiant of intermediate and late (cooler) spectral type. It shows...

24 Cephei is a single, yellow-hued star in the northern circumpolar constellation of Cepheus. With an apparent visual magnitude of 4.79, it is faintly...

While(1<2) 5:29 11. "Fn Pig" (ov) Album Title Goes Here 8:32 12. "HR 8938 Cephei" (ov) non-album single 5:52 13. "Superbia" (ov) While(1<2) 4:23 14. "Caritas"...

HD 221525 is a single star near the north celestial pole in the constellation Cepheus. At an apparent magnitude of 5.56, it can be seen with the naked...

their spectra. The primary is a blue giant and a variable star of the Beta Cephei type. Spica, along with Arcturus and Denebola—or Regulus, depending on the...

the pole will begin to move away. It will pass by the star Errai (Gamma Cephei) in 4000 AD, Deneb in 10,000 AD, and Vega in 14,500 AD. The celestial pole...

Size comparison of Betelgeuse, Mu Cephei, KY Cygni, and V354 Cephei according to Emily Levesque's publication...

7 Cephei is a single star located approximately 820 light years away, in the northern circumpolar constellation of Cepheus. It is visible to the naked...

examples of stars in this mass range include Antares, Spica, Gamma Velorum, Mu Cephei, and members of the Quintuplet Cluster. Type Ia supernova progenitors are...

G8: β Aquilae, δ Pavonis, λ Andromedae K0: η Cephei, κ Coronae Borealis, δ Eridani, 55 Cancri A K1: γ Cephei, π Hydrae, φ Serpentis, δ Leporis Later analysis...

stellar association Cepheus OB2, located one degree south-southwest of VV Cephei. NGC 7160 is a young cluster, whose age is estimated to be between 10 and...

closer to Alrai (Gamma Cephei). In about 5,500 years, the pole will have moved near the position of the star Alderamin (Alpha Cephei), and in 12,000 years...

Cephei MY Cephei NML Cygni NR Vulpeculae PZ Cassiopeiae RT Carinae RW Cygni S Persei Stephenson 2 DFK 1 UY Scuti V602 Carinae V1749 Cygni VV Cephei A...

and a few months later by John Goodricke with the variability of Delta Cephei, the eponymous star for classical Cepheids. Most of the Cepheids were identified...

to glow with a blue-white hue. Delta Crucis is a strong candidate Beta Cephei variable. Its rotation is very fast, with a projected rotational velocity...

the detection of pulsations, the Aa component has been classified as a β Cephei variable. Beta Centauri is well known in the Southern Hemisphere as the...

/ælˈnaɪjæt/, the traditional name for the entire star system) and a Beta Cephei variable) and Aa2; a third component (designated Sigma Scorpii Ab) at 0...

cool supergiants and hypergiants such as V509 Cassiopeiae (HR 8752) and RW Cephei. "Ass Cep OB 1". SIMBAD. Centre de données astronomiques de Strasbourg....

Charana cepheis, also known as the Cachar mandarin blue is a butterfly in the family Lycaenidae. It is found in Assam, Bangladesh, Myanmar and north Vietnam...

radiated by the star in the visible spectrum). Henrietta found that Delta Cephei was the "standard candle" that had long been sought by astronomers. A similar...

estimated diameter of VV Cephei A, a red hypergiant with a blue dwarf companion. 1.75 Tm – 11.7 au – estimated diameter of Mu Cephei, a red supergiant (possibly...

star. Alpha Muscae appears to be a Beta Cephei variable star. Telting and colleagues report it as a Beta Cephei with a high degree of confidence as they...

ten variable stars were known. John Goodricke himself discovered Delta Cephei and Beta Lyrae. Since 1850, the number of known variable stars has increased...

16 Cephei is a single star located about 119 light years away from the Sun in the constellation of Cepheus. It is visible to the naked eye as a faint,...

"Analysis of far-infrared fine-structure emissions from the red supergiant μ Cephei". Astronomy & Astrophysics. doi:10.1051/0004-6361/202660113. ISSN 0004-6361...

two B-type stars and a pre-main-sequence star. The primary star is a Beta Cephei variable star with rapid brightness changes of about a hundredth of a magnitude...

the existence of a substellar companion to Gamma Cephei was suspected since 1988, the planet Gamma Cephei Ab was not confirmed until 2003, and that is listed...

range from 4 to 11.9 million years. At the center of the cluster lies DH Cephei, a close, double-lined spectroscopic binary system consisting of two massive...

peculiarity of numerous bright lines. It appears similar to the spectrum of VV Cephei (HR 8383), an eclipsing binary. P. Swings and O. Struve in 1941 discovered...

former Ukrainian airline v/v (volume by volume), the volume fraction VV Cephei, a star system Vorontsov-Vel'yaminov Interacting Galaxies, a catalogue of...

sequence star with variable spectral lines, it was suspected of being a β Cephei variable but this classification was repeatedly rejected. The short-period...

2.25 billion years old. This star is occasionally known as Upsilon Cephei (υ Cephei). According to the Bright Star Catalogue, this Bayer designation appeared...

The system is a member of the young open cluster NGC 6871 and exhibits β Cephei type pulsations in its primary component, making it a key object for studying...

hotter K types, are sometimes described as orange supergiants (e.g. Zeta Cephei), or even as yellow (e.g. yellow hypergiant HR 5171 Aa).[citation needed]...

a doctorate in astronomy in 1962. His thesis was titled "The system VV cephei," and his doctoral advisor was Dean Benjamin McLaughlin. His thesis work...

B2Ia Omicron² Canis Majoris, B-type supergiant, spectral type B3Ia Lambda Cephei, O-type supergiant, spectral type O6.5I(n)fp Mu Sagittarii, B-type supergiant...

standards: B0V – Upsilon Orionis B0Ia – Alnilam B2Ia – Chi2 Orionis B2Ib – 9 Cephei B3V – Alkaid B3V – Eta Aurigae B3Ia – Omicron2 Canis Majoris B5Ia – Eta...

day)", although this terminology is rarely seen elsewhere. The similar Beta Cephei variables have shorter periods and have p-mode pulsations, while the SPB...

809 TOI-1518 TOI-2267 WISE 0313+7807 WR 156 ZTF J1239+8347 Exoplanets γ Cephei Ab (Tadmor) TOI-1431 b Star clusters NGC 188 6939 7023 7055 7129 7142 7160...

times the mass of the Sun and 6.4 times the Sun's radius. It is a Beta Cephei type variable star with a brightness that periodically varies from magnitude...

allowing freer travel to the Western world. The first extrasolar planet, Gamma Cephei Ab (confirmed in 2003), was detected this year and the World Health Organization...

other heavily mass-losing hypergiant stars, such as VY Canis Majoris, Mu Cephei, and the post-red supergiant IRC +10420. A much lower luminosity of 280...

Majoris was called Oupo by the people of the Tuamotus. Mirzam is a Beta Cephei variable that varies in apparent magnitude between +1.97 and +2.01 over...

can be seen among the stars of the constellation Cepheus. The star Zeta Cephei is specifically named after him. A famous presentation of the story is available...

Spica, Rigel and Deneb, the red supergiants Betelgeuse, Antares, and VV Cephei A; the yellow hypergiant Rho Cassiopeiae; the luminous blue variable Eta...

star the blue-white hue that is typical of B-type stars. It is also a Beta Cephei variable star with a primary pulsation period of 0.1603 days, or 6.24 cycles...

Campbell, Bruce; Yang, Stephenson (2003-12-20). "A Planetary Companion to γ Cephei A". The Astrophysical Journal. 599 (2): 1383–1394. arXiv:astro-ph/0305110...

(2023-07-01). "Solar-like oscillations in γ Cephei A as seen through SONG and TESS - A seismic study of γ Cephei A". Astronomy & Astrophysics. 675: A197....

to their large size. Red supergiants like Betelgeuse, Antares, Mu Cephei, VV Cephei, and VY Canis Majoris one of the biggest stars in the Universe, are...

Australis Past and future Northern Vega Tianbang Asuusiha Thuban Kochab Errai ι Cephei Alfirk Alderamin Deneb Fawaris Southern β Hydri γ Chamaeleontis I Carinae...

in the family Lycaenidae. Charana mandarinus (Hewitson, 1863) Charana cepheis de Nicéville, 1894 Assam Wikimedia Commons has media related to Charana...

a Beta Cephei variable. (At the time he actually identified it as a Beta Canis Majoris star, which was subsequently designated a Beta Cephei variable...

or B3 star several times hotter than the Sun. HD 148703 is a candidate β Cephei variable and its variability was first noticed in 1983 by C. Sterken. Further...

2022, the array was used to observe the disc of the hypergiant star RW Cephei during its ongoing dimming event. CHARA holds annual science meetings where...

(Edasich) 101.2 ± 0.3 Draco 15h 24m 55.77463s +58° 57′ 57.8344″ K2III 3.290 Xi Cephei (Kurhah) Ba 101.34 ± 0.06 Cepheus 22h 03m 47.440s +64° 37′ 40.70″ A3Vm 4...

Space Telescope: A Parallax of the Fundamental Distance Calibrator delta Cephei". The Astronomical Journal. 124 (3): 1695–1705. arXiv:astro-ph/0206214....

Scorpii. Many of them are variable stars, mostly pulsating Cepheids such as δ Cephei itself. Hertzsprung–Russell diagram Spectral type O B A F G K M L T Brown...

809 TOI-1518 TOI-2267 WISE 0313+7807 WR 156 ZTF J1239+8347 Exoplanets γ Cephei Ab (Tadmor) TOI-1431 b Star clusters NGC 188 6939 7023 7055 7129 7142 7160...

with a stellar classification of B3 Ib. It has been classified as a Beta Cephei type variable star, but the supergiant spectral type and a period of over...

Sun. The primary component of this system is a variable star of the Beta Cephei type with a period of just 3h 22m. It has an estimated 8.0 to 8.6 times...

of the Pier Aeromar (former IATA code: VW), a former Mexican airline VW Cephei, a binary star system VW Hamme or VW Hamme, a Belgian association football...

uncertain. This group contains about 16 stars, including Alpha Librae, Alpha Cephei, Castor, Fomalhaut and Vega. All members of the group are moving in nearly...

astronomer, who identified Algol as an eclipsing variable and discovered δ Cephei MPC · 3116 3117 Niépce 1983 CM1 Joseph Nicéphore Niépce, 18th–19th-century...

5m.50 0.50   Zeta Ophiuchi Ophiuchus 2m.56 2m.58 0.02 O9.5V Also a Beta Cephei variable Pleione Taurus 4m.77 5m.5 0.77 B8Vne Lambda Pavonis Pavo 4m.00...

notably includes evolved blue and red supergiants such as Nu Cephei, Mu Cephei, and VV Cephei. In particular, it is surrounded by a loose cluster of stars...

difficult to detect. Other classes of unstable main-sequence stars, like Beta Cephei variables, are unrelated to this instability strip. The total amount of...

Infrared image of RSGC1 cluster by Spitzer, with 2MASS image inset Mu Cephei NML Cygni Stephenson 2 DFK 1 – mistakenly referred to as "RSGC1-01" in a...

variables: NV Puppis is a Gamma Cassiopeiae variable, while NW Puppis is a Beta Cephei variable. "Cl Collinder 135". SIMBAD. Centre de données astronomiques de...

(Ptolemy) centaur Alpha Centauri −0.27 1060 Cepheus /ˈsiːfiəs/ Cep Ceph Cephei /ˈsiːfiaɪ/ ancient (Ptolemy) Cepheus (mythological character) Alderamin...

unconfirmed exoplanets. SSSPM J1549-3544 313.2 ± 0.6 Lupus sdK5 14.78 Kappa Cephei 314 Cepheus B9III TOI-3493 315.59±0.65 G0 Has one known exoplanet. HD 108501...

31.008s –01° 04′ 23.68″ 1090 Possibly eclipses by circumstellar dust RW Cephei K2 0-Ia 6.0–7.6 — 22h 23m 07.01521s +55° 57′ 47.6244″ 11,000 Great dimming...

index +0.55 B−V color index +0.70 R−I color index +0.48 Variable type δ Cephei Astrometry Radial velocity (Rv) +7.2 km/s Proper motion (μ) RA: +0.800 mas/yr...

published for other supergiant stars, such as VX Sagittarii, NML Cygni, MY Cephei, and Stephenson 2 DFK 1. In addition, other leading candidates have been...

are α and 4 Lacertae, π2 and π1 Cygni, stars 5 and 6, HD 206267, 13 and ε Cephei, β Lacertae, σ, ρ, τ, and AR Cassiopeiae, 9 Lacertae, 3, 7, 8, λ, ψ, κ,...

Australis Past and future Northern Vega Tianbang Asuusiha Thuban Kochab Errai ι Cephei Alfirk Alderamin Deneb Fawaris Southern β Hydri γ Chamaeleontis I Carinae...

GitHub project Kaldi paper - The Kaldi Speech Recognition Toolkit VOSK – open source and commercial models from Alpha Cephei on Kaldi foundations v t e...

the constellation Puppis. Anamarija Stankov confirmed this star as a Beta Cephei variable. Analysis of its spectrum and allowing for extinction gives a mass...

Zhao; et al. (2009). "Imaging And Modeling Rapidly Rotating Stars: Alpha Cephei And Alpha Ophiuchi". The Astrophysical Journal. 701 (1): 209–224. arXiv:0906...

Spectral type bow shock aligned/not aligned with star motion Belongs to Alpha Cephei 15.04 A8Vn not aligned Beta Librae 56.75 B8Vn not aligned Mimosa 85.40 B1IV...

Henry Draper Catalogue (HD) are HD 126357 and 126449. HD 126357 is a Beta Cephei variable, and the cluster also contains two pulsating variables, CD-59 5259...

rim being illuminated by HD 206267. The red supergiant or hypergiant Mu Cephei is located at the edge of the nebula. It is well known for being one of...

Linux/Binom Bliss – requires root privileges Brundle Bukowski Caveat Cephei – Linux.Cephei.A (and variants) Coin Hasher Lacrimae (a.k.a. Crimea) Nuxbee – Virus...

mixed traits of a main sequence star and a subgiant. It is a suspected Beta Cephei variable or a slowly pulsating B star. The star has about nine times the...

Zimmerman also released two non-album singles; "Aural Psynapse" and "HR 8938 Cephei", and was nominated for his third Grammy for a remix of the song "Rope"...

caledonica (C. & R. Felder, [1865]) New Caledonia Nothodanis schaeffera cepheis (Druce, 1891) Solomon Islands Nothodanis schaeffera esme (Grose-Smith,...

astronomer Gerard Kuiper, including: KUI 91AB, a variable star of Delta Cephei type KUI 93AB, an eclipsing binary of Algol variable type Kui (Chinese mythology)...

terms of slow changes in the pulsar's dispersion measure". 51 Pegasi Gamma Cephei Ab List of exoplanets discovered before 2000 - Draugr, Poltergeist and Phobetor...

B-type main-sequence star has a stellar classification of B1 V. It is a Beta Cephei variable, ranging from 5.01 to 4.96 magnitude with a period of 0.19 days...

refer to three different stars in the constellation Puppis: X Puppis, a δ Cephei variable X Puppis, (HR 2548, 38 G. Puppis) an F-type main-sequence star...

main uncertainties affecting theoretical modeling. β Cephei stars: Seismic analyses of β Cephei stars show that it is not obvious to derive a one-to-one...

Alfirk β Cephei Aa Cepheus Arabic From Arabic: الفرق al-firq ('the flock'). Name given by Ulugh Beg to the asterism consisting of α, β and η Cephei. /ˈælfərk/...

7.7 V553 Centauri, 8.2 SW Tauri, 9.3 RT Trianguli Australis, 9.4 V351 Cephei, 9.5 BL Herculis. 9.7 BD Cassiopeiae, 10.8 UY Eridani, 10.9 The BL Herculis...

1,300 light-years distant from the Solar System. It is a suspected Beta Cephei variable. Located south of Iota Orionis, Upsilon Orionis is one of two stars...

Stankov, Anamarija; Handler, Gerald (June 2005), "Catalog of Galactic β Cephei Stars", The Astrophysical Journal Supplement Series, 158 (2): 193–216,...

59.5s +57° 41′ 45″ M3.0V 0.271 9.79 11.76 249.5 ±0.1 B flare star B (DO Cephei) M4.0V 0.176 11.41 13.38 DENIS J1048−3956 13.1932 ±0.0027 Ant* 10h 48m 14...

in Cygnus; and Delta Cephei (itself the prototype) and Polaris are Cepheid variables and yellow supergiants. Antares and VV Cephei A are red supergiants...

Binary star system 2.45 2.38 Eta Canis Majoris (Aludra) Star 2.46 Alpha Cephei (Alderamin) Star Suspected variable star 2.473 Kappa Velorum (Markeb) Binary...

star that is currently fusing its core hydrogen. It is a suspected Beta Cephei variable star. It was one of the first O-type stars (along with S Monocerotis)...

star of magnitude 1.3, and lies 353 light-years from Earth. It is a Beta Cephei-type variable star with a variation of less than 0.1 magnitudes. γ Crucis...

45 ± 2 03h 04m 48.95s −27° 05′ 13.35″ Y0pec WISE 2226+0440 45.0 T8 Gamma Cephei (Errai) A$ 45.0 ± 0.3 Cepheus 23h 39m 20.910s +77° 37′ 56.51″ K1IVe 3.22#...

Canis Majoris. Also called Mirzam or Murzim, Beta is a blue-white Beta Cephei variable star of magnitude 2.0, which varies by a few hundredths of a magnitude...

possibility of Beta Lupi becoming a white dwarf. This is a multi-period Beta Cephei variable with a dominant oscillation period of 0.232 days. It is a proper...

Commons Quotations from Wikiquote Resources from Wikiversity Galileo to Gamma Cephei – The History of the Telescope. Archived 8 May 2013 at the Wayback Machine...

estimated mass of 1,937 M☉, of which about 24% is interstellar matter. A Delta Cephei type variable star designated U Sagittarii is a member of this cluster,...

87 2.45 Aludra η Canis Majoris 2,000 B5 Ia Southern 88 2.46 Alderamin α Cephei 49 A8Vn Northern 89 2.46 Markeb κ Velorum 0540 B2 IV Southern 90 2.47 (1...

imperial Neocheritra fabronia 1 Schedule 2 Cachar mandarin blue Charana cepheis Schedule 1 Mandarin blue Charana mandarina 1 Red imperial Suasa lisides...

bound, yellow hypergiants and red supergiants are not clearly separated; RW Cephei (roughly 4,000 K (3,730 °C; 6,740 °F), 295,000 L☉) is an example of a star...

Size comparison of some well-known supergiant and hypergiant stars, featuring Cygnus OB2-12, V382 Carinae, Betelgeuse, VV Cephei, and VY Canis Majoris...

disc that formed after the death of the white dwarf's progenitor. Gamma Cephei and Nu2 Canis Majoris, another similar-sized giant stars hosting a jovian...

Verteilung der Veränderlichen vom δ Cephei-Typus" [On the spatial distribution of variable [stars] of the δ Cephei type]. Astronomische Nachrichten (in...

parsecs from Earth in the constellation of Cepheus, centred around the star β Cephei. It is about 100 parsecs above the galactic plane of the Milky Way galaxy...

SiO maser emission. TZ Cassiopeiae PZ Cassiopeiae List of largest stars T Cephei Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation"...

In the sky it positioned just to the west of the magnitude 3.2 star Beta Cephei (β Cep). This object has a yellow hue similar to the Sun but is too faint...

giving it the blue-white hue of a B-type star. It was a suspected Beta Cephei variable, until observations with TESS led to its classification as a slowly...

Cepheids W Virginis Delta Scuti RR Lyrae Mira Semiregular Irregular Beta Cephei Alpha Cygni RV Tauri Eruptive variables Flare stars T Tauri FU Orionis RCr...

their mythical beings. Not far away was the Martian North pole star, Delta Cephei, which is a variable star. Its changing brightness was likened to the breathing...

the naked eye. It has a stellar classification of B1.5III and is a Beta Cephei variable. This star has more than ten times the mass of the Sun and is more...

809 TOI-1518 TOI-2267 WISE 0313+7807 WR 156 ZTF J1239+8347 Exoplanets γ Cephei Ab (Tadmor) TOI-1431 b Star clusters NGC 188 6939 7023 7055 7129 7142 7160...

S2CID 118403321. McClure, Bruce; Byrd, Deborah (22 September 2021). "Gamma Cephei, aka Errai, a future North Star". earthsky.org. Retrieved 25 December 2021...

about 690 light-years from the Sun. Since a member of the system is a β Cephei-type variable star, the magnitude is not fixed but varies slightly between...

the designation for the 15th variable star named in a constellation: RW Cephei, an orange hypergiant located in the constellation Cepheus RW Cygni, a red...

giving it the blue-white hue of a B-type star. It is classified as a Beta Cephei type variable star with a primary period of 0.16961 days (4 hours 4 minutes)...

radial-velocity observations suggested that a planet orbits the star Gamma Cephei. Partly because the observations were at the very limits of instrumental...

acquisitions. Cephei Capital was founded in 2006 with the support from CDH. Cephei focuses on investing in Chinese companies in the secondary market. Cephei now...

Scorpius, 3,000 light years away. The primary is a Classical Cepheid (δ Cephei) variable and its visual magnitude varies from 6.4 to 6.9. V636 Scorpii...

mass-loss, similar to those of Betelgeuse and RW Cephei. The rebrightening of B90, just like RW Cephei, took twice as long as that of Betelgeuse which...

variables, rapidly oscillating Ap stars (roAp) and ZZ Ceti variables. In Beta Cephei variables, stellar pulsations occur at a depth where the temperature reaches...

(1946). "The observations of brightness, colour and radial velocity of δ Cephei and the pulsation hypothesis (Errata: 10 258, 310)". Bulletin of the Astronomical...

809 TOI-1518 TOI-2267 WISE 0313+7807 WR 156 ZTF J1239+8347 Exoplanets γ Cephei Ab (Tadmor) TOI-1431 b Star clusters NGC 188 6939 7023 7055 7129 7142 7160...

also known as 2M1207b. Iota Aquarii 211 ± 3 Aquarius B8 V 4.279 Omicron Cephei A 211 ± 7 Cepheus G8III 4.86+7.13 B F6V Gamma Gruis (Aldhanab) 211 ± 9 Grus...

l-Yamīn the Right Arm (of Cepheus) الذراع اليمين الذّراع اليَمِين Alpha Cephei Aldhibah ʼaḍ-Ḍibaāʽ [Adh-Dhibaaʽ], ʼaḍ-Ḍibāʽ [Adh-Dhibaaʽe] the Hyenas الضباع...

pulsating variable candidate showing characteristics associated with both Beta Cephei variable and 53 Persei variable stars. It lies in the faint equatorial constellation...

Retrieved 20 August 2010. "Telescope History: Sky High — Galileo to Gamma Cephei". McDonald Observatory. 1990-04-24. Archived from the original on 30 March...

nonradial pulsations in the Delta Scuti stars Delta Delphini and Epsilon Cephei", Astronomy and Astrophysics, 269 (1–2): 195–200, Bibcode:1993A&A...269...

14256825 A 2,700 ± 100 2 sdOB 13.2 Has a M-type companion star. Lambda Cephei 3,098.5 1 O6.5If(n)p +5.050 HD 193322 3,100 2 O9Vnn + O8.5 III +5.958 Mu...

constellation Ara, lying close to the galactic equator. It contains one β Cephei variable. Kharchenko, N. V.; et al. (August 2005). "Astrophysical parameters...

method, but later detected using astrometry, e.g. Epsilon Indi Ab or Gamma Cephei Ab. This list contain only confirmed planets. Many candidate planets were...

Eri is classified in the General Catalogue of Variable Stars as a Beta Cephei variable. The AAVSO International Variable Star Index defines a LERI type...

even larger red supergiants, such as VY Canis Majoris, KY Cygni, RW Cephei or Mu Cephei. Antares, like the similarly sized red supergiant Betelgeuse in the...

what gives it the blue-white hue of a B-type star. It is a candidate Beta Cephei variable that shows line-profile variations in its spectrum. However, the...

telescope, it is a pulsating star that displays characteristics of a Beta Cephei variable, a slowly pulsating B-type star, and a rotating variable. It is...

eclipsing binary. Next to it is BV Cru, a magnitude 8.662 B0.5 giant and Beta Cephei variable. Next in line is DU Cru, an M2 red supergiant that varies irregularly...

203664 105614 21h 23m 28.81s +09° 55′ 54.9″ 8.53 -2.02 4200 B0.5IIIn Beta Cephei variable, Vmax = 8.520m, Vmin = 8.585m, P = 0.1658677 d R Equ R 202051 21h...

consisting of a red supergiant and a small hot companion, similar to VV Cephei. The companion has been identified from a high excitation component in the...

been identified as part of the group include Castor, Fomalhaut, Vega, α Cephei and α Librae. While the reported group members are young (typically with...

times as luminous and 8 times as massive as the Sun. The star is a Beta Cephei variable with about 4.7 times the Sun's diameter, and pulsates every 2.2 hours...

non-GCAS Be star variables. λ Eridani itself is incorrectly listed as a Beta Cephei variable. The AAVSO International Variable Star Index defines a LERI type...

O8 types, and listed 5 O9 V standards (HD 46202, HD 52266, HD 57682, 14 Cephei, 10 Lacertae) and 3 O9.5 V standards (HD 34078, Sigma Orionis, Zeta Ophiuchi)...

direction. Among the brightest stars belonging to this group is Lambda Cephei, which with its magnitude of 5.05 is visible even to the naked eye, provided...

the blue-white glow of a B-type star. In 1956 it was identified as a Beta Cephei variable by Bernard Pagel and colleagues, which means it undergoes periodic...

Be star and NGC 6910 14 and NGC 6910 25 are beta Cephei variables. In total there are four beta Cephei variables in the cluster, a rather high number....

"International observational campaigns of the last two eclipses in EE Cephei: 2003 and 2008/9". Astronomy and Astrophysics. 544: A53. arXiv:1205.0028...

compared to a critical velocity of 389 km/s. The star appears to be a Beta Cephei variable with a pulsation period of 0.0919 days and an amplitude of 0.0080...

Gamma Cephei, Psi Draconis, 16 Draconis, Psi Herculis, Kappa Coronae Borealis and Delta Coronae Borealis. The object stopped near Gamma Cephei at an azimuth...

Cepheid variables. Using these relations the distance is calculated to delta Cephei, and compared with an independent distance derived from trigonometric parallax...

Tite, 1963 Prosotas dubiosa livida Tennent, 2000 Nothodanis schaeffera cepheis (Druce, 1891) Catopyrops ancyra amaura (Druce, 1891) Catopyrops ancyra...

Draconis, ι Draconis, η Draconis, ζ Draconis, υ Draconis, 73 Draconis, γ Cephei and 23 Cassiopeiae. Consequently, the Chinese name for θ Draconis itself...

titled A Spectrophotometric Study of the Cepheid Variables η Aquilae and δ Cephei. The measurements he got were 3 times larger than theoretically possible...

was a magnitude 8.0 object about 3 degrees southeast of the star Kappa Cephei. The subsequent two nights were clear, which helped Candy and G. E. Taylor...

Draconis, ι Draconis, η Draconis, ζ Draconis, θ Draconis, 73 Draconis, γ Cephei and 23 Cassiopeiae. This is a single-lined spectroscopic binary star system...

C.; Henrichs, H. F. (2006). "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars". Astronomy and Astrophysics. 452 (3): 945. Bibcode:2006A&A...

variations of this star in 1938 led to it being incorrectly classified as a Beta Cephei-type star, although there was some early disagreement about the variation...

during a blue loop from the red-giant branch, are thought to make up the δ Cephei variables. Both types of star have luminous and unstable photospheres at...

S2CID 14878976. Percy, J. R.; Lane, M. C. (May 1977). "Search for Beta Cephei stars. I - Photometric and spectroscopic studies of northern B-type stars"...

shows regular variation in luminosity of the type that occurs with Beta Cephei variables, at a periodicity of 10.36 cycles per day. This star system is...

(zēng yī, 1st added star), 增二 (zēng èr, 2nd added star) etc. For example, γ Cephei is referred to as 少衛增八 (Shào Wèi Zēng Bā, 8th Added Star of Second Imperial...

the long period variable AGB stars. At hotter temperatures are the Beta Cephei and PV Telescopii variables. Right at the edge of the instability strip...

Light curve of δ Cephei showing magnitude versus pulsation phase...

of β Lacertae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae...

will become the "north star". In approximately 3,200 years, the star Gamma Cephei in Cepheus will next succeed the other star which has great apparent magnitude...

Delta (Sarvvis) Psi (4.3), and 48 Persei (4.0);, the 2.9 magnitude Beta Cephei variable Epsilon Persei (Áldu) and the stars 29 (5.2), 30 (5.5), 31 (5.0)...

Lowater's spectrographic research examined Mira, R Leonis, R Serpentis, and T Cephei and studied the absorption spectra of sulfur dioxide. Her research was conducted...

consisting of α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae...

B1.5 III that is 460 ± 10 light-years distant from Earth. It is a Beta Cephei variable, pulsating in brightness by 0.03 of a magnitude every 7 hours and...

Eggen, O. J. (1971). "The zeta Herculis, sigma Puppis, ε Indi, and eta Cephei Groups of Old Disk Population Stars". Publications of the Astronomical Society...

the I Lacertae OB association (Lac OB1). The primary component is a Beta Cephei variable with a stellar classification of B1.5III, matching a B-type star...

brightness variability has led to the star being classified as a pulsating Beta Cephei variable, but no evidence has been found of pulsations superimposed on the...

J2339–0424 291 ± 2 DABZ Alpha Vulpeculae (Anser) 291 ± 3 Vulpecula M1 III 4.40 V Cephei 291.6 ± 0.7 Cepheus A1V 6.57 Zeta Apodis 293 ± 3 Apus K2 III +4.78 HD 48265...

Light curve of a Delta Cephei variable, showing the regular light curve formed by intrinsic stellar pulsations...

(also called Hind's Variable Nebula), and discovered the variability of μ Cephei. Hind discovered Nova Ophiuchi 1848 (V841 Ophiuchi), the first object of...

Puppis by Lacaille, reassigned to Carina as A Carinae by Gould Upsilon Cephei was designated to the star HR 7955 that appeared in Burritt's star atlas...

Hubrig, S.; et al. (April 2009). "New magnetic field measurements of β Cephei stars and slowly pulsating B stars". Astronomische Nachrichten. 330 (4):...

 181–184. ISBN 978-1-85109-665-7. Malatesta, Kerri (16 July 2010). "Delta Cephei". American Association of Variable Star Observers. Clark, David H.; Matthew...

effective temperature of 26,530 in its outer atmosphere. Omega1 Scorpii is a β Cephei star that undergoes non-radial pulsations at a rate of 15 cycles per day...

The primary component of the pair, κ Sco A, is a variable star of Beta Cephei type. It is undergoing radial pulsations with a dominant frequency of five...

variable", later called a Cepheid variable after the prototype star Delta Cephei, showed a definite relationship between the variability period and the star's...

371L. doi:10.1086/190179. Hilditch, R. W. (1974). "The binary systems 14 Cephei and 2 Lacertae". Monthly Notices of the Royal Astronomical Society. 169...

star was classified as a hybrid slowly pulsating B-type star and a Beta Cephei variable. Both g (gravity) and p (pressure) mode pulsations were detected...

1981, listed in the General Catalogue of Variable Stars as a possible δ Cephei variable. It has been described as a pseudo-Cepheid, a supergiant with pulsations...

with those of red supergiants. AH Scorpii BC Cygni HV 11423 IRC −10414 MY Cephei NML Cygni S Persei Stephenson 2 DFK 1 VY Canis Majoris Westerlund 1 W26...

Australis Past and future Northern Vega Tianbang Asuusiha Thuban Kochab Errai ι Cephei Alfirk Alderamin Deneb Fawaris Southern β Hydri γ Chamaeleontis I Carinae...

white dwarf-pulsar binary PSR B1620-26, the subgiant-red dwarf binary Gamma Cephei, and the white dwarf-red dwarf binary NN Serpentis, among others. A study...

The binary HD 300933/4 is a probable VV Cephei-type star with a composite spectrum similar to that of V381 Cephei (HR 8164), but with weaker emission lines...

809 TOI-1518 TOI-2267 WISE 0313+7807 WR 156 ZTF J1239+8347 Exoplanets γ Cephei Ab (Tadmor) TOI-1431 b Star clusters NGC 188 6939 7023 7055 7129 7142 7160...

over 10th magnitude, with five known to be variable. A total of four β Cephei-type variables have been identified, one of the highest such totals for...

365H. Duncan, J. C.; Mitchell, H.M. (1929). "The radial velocity of beta Cephei on August 21, 1928". Astrophysical Journal. 70: 127–130. Bibcode:1929ApJ...

Cassiopeiae variable and spectroscopic binary υ2 Puppis (NW Puppis), a β Cephei variable Neither component of this double is given a letter in Lacaille's...

electronics Sahara (1991) for orchestra Dunas (1991) for string orchestra Delta Cephei (1991) for 2 clarinets, violin, viola and violoncello Rigel (1993) for electronics...

radial velocity of +13 km/s. This star was originally thought to be a Beta Cephei variable and a suspected eclipsing binary with an orbital period of 133...

Johnson, H. L. (1959). "Photoelectric Photometry of the Association III Cephei". The Astrophysical Journal. 130: 69. Bibcode:1959ApJ...130...69B. doi:10...

corner of Cepheus. The open cluster is located two degrees southwest of Eta Cephei and 2/3° northwest from the spiral galaxy NGC 6946, which has visual magnitude...

Observations with the CHARA Array. II. omega Andromeda, HD 178911, and xi Cephei" (PDF). The Astronomical Journal. 148 (3). 48. arXiv:1407.0639. Bibcode:2014AJ...

warrior Memnon. The earlier detection of the planets HD 114762 b and Gamma Cephei Ab was considered uncertain at the time and so they are not considered the...

Crucis is listed in the General Catalogue of Variable Stars as a possible β Cephei-type variable. Its brightness varies with an amplitude of 0m.02 over a period...

most luminous galactic red supergiants, which includes V354 Cephei, KY Cygni and Mu Cephei. In 2011, its bolometric luminosity was re-measured to be at...

Ignace, R.; Hamann, W.-R.; Balona, L. (2015). "On X-ray pulsations in β Cephei-type variables". Astronomy & Astrophysics. 577: A32. arXiv:1503.05749. Bibcode:2015A&A...

one of the reddest naked-eye stars in the night sky, second only to Mu Cephei (the Garnet Star). 119 Tauri is classified as a semiregular variable star...

Retrieved 30 April 2022. Jakate, S. M. (April 1979). "A search for Beta Cephei stars. III. Photometric studies of southern B-type stars". Astronomical...

vary between magnitudes 5.06 and 5.17 in 1960. It was classified as a Beta Cephei variable in the Hipparcos and Tycho Catalogues (ESA 1997), with a period...

occults Regulus. c. 5200 Due to axial precession, ι Cephei will replace the previous target, γ Cephei, as Earth's northern pole star (the next naked eye...

im Spectrum von δ Cephei, 1913 (Izv. GAO, vol. 5, no. 59). Ueber die relative Intensitätsäinderung der Linien im Spectrum von δ Cephei und S Gemin., 1914...

star as a giant combined with an underestimation of the orbit of the Gamma Cephei binary, which implied the planet's orbit would be unstable, led some astronomers...

2014/3/12 293 Yue Xiu Asset Management Limited United States 2014/3/19 294 Cephei Capital Management (Hong Kong) Limited Hong Kong 2014/3/26 295 Overlook...

Musalsalah in Arabic. It has also been called Persea ("Perseus's wife") or Cepheis ("Cepheus's daughter"), all names that refer to Andromeda's role in the...

Spectral type Comment γ Boötis (Seginus) 3.02 3.07 0.05 6.96 h A7III ε Cephei 4.15 4.21 0.06 0.98 h F0IV HD 40372 5.88 5.92 0.04 1.466 h A5me In eclipsing...

19 – John Goodricke begins his observations of the variable star Delta Cephei from York. Publication of the Annals of Agriculture edited by Arthur Young...

Desmet, M.; Aerts, C. (November 2006). "An asteroseismic study of the β Cephei star β Canis Majoris". Astronomy and Astrophysics. 459 (2): 589–596....

satellite has shown that one of the stars in the α Crucis system is a β Cephei variable, although α1 and α2 Crucis are too close for TESS to resolve and...

; et al. (August 2009). "Imaging and Modeling Rapidly Rotating Stars: α Cephei and α Ophiuchi". The Astrophysical Journal. 701 (1): 209–224. arXiv:0906...

ESA Giotto July 1988 First suspected detection of an exoplanet (Gamma Cephei Ab). Canada Astronomers Bruce Campbell, Gordon Walker and Stephenson Yang...

stars. Markab has an apparent magnitude of 2.48, while Algenib is a Beta Cephei variable that varies between magnitudes 2.82 and 2.86 every 3 hours 38 minutes...

Astronomical Society by Canadian astronomer, Robert Methven Petrie. It is a Beta Cephei variable that ranges between magnitudes 6.44 and 6.68 over a period of 4...

eclipse of the primary component has been detected. This component is a Beta Cephei variable star with three dominant pulsation modes having frequencies of...

M3-4 + M5-6 b 902 HD 222237 Tucana 37.329 ± 0.008 7.09 K3+V b 903 Gamma Cephei (Errai) Cepheus 44.98 ± 0.09 3.21 K1III-IV CN1 + M4V Ab (Tadmor) 904 Iota...

Hubrig, S.; et al. (January 2009), "New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars", Astronomische Nachrichten, 330 (4):...

that of the Sun and has a surface temperature of 21,429 K. It is a Beta Cephei variable. A magnitude 5.7 star, it will be faintly visible on moonless nights...

Goodricke is credited with discovering the periodic variation of β Lyrae and δ Cephei, the prototypical example of the Cepheid variable stars. Although several...

79 43 — — — 100 — — 9 — "Bad Selection" — — — — — 137 — — 16 — "HR 8938 Cephei" 2011 — — — — — — — — — — Non-album single "Raise Your Weapon" (featuring...

official standing with the International Astronomical Union. 51 Pegasi b Gamma Cephei Ab Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical...

material around it. Binaries with such a characteristic are referred to as VV Cephei systems, although in this case the components do not eclipse each other...

Canis Majoris, one of the largest stars and galactic red supergiants Mu Cephei, possibly one of the largest galactic red supergiants BAT99-98, one of the...

α Geminorum Ba 2.96 α Volantis 4.00 Acubens A α Cancri A 4.26 Kurhah ξ Cephei 4.29 θ1 Crucis 4.30 π Virginis 4.64 μ Aurigae 4.88 2 Ursae Majoris 5.46...

S2CID 255195566. Hoffmeister, Cuno (May 1957), "On Two Abnormal Stars of Delta Cephei Type", Astrophysical Journal, 125: 824, Bibcode:1957ApJ...125..824H, doi:10...

(July 2023). "Solar-like oscillations in γ Cephei A as seen through SONG and TESS: A seismic study of γ Cephei A". Astronomy & Astrophysics. 675: A197....

stellar classification of B3V. It has been classified as a candidate Beta Cephei variable with a period of 2.2 days, although this designation was rejected...

the northern constellation of Cygnus, abbreviated X Cyg. This is a Delta Cephei variable that ranges in brightness from an apparent visual magnitude of...

Zehev Tadmor Israeli chemical engineer Tadmor (planet), the exoplanet Gamma Cephei Ab All pages with titles containing Tadmor All pages with titles containing...

resulting in a rotational period of 13 to 17 days. β Crucis A is a known β Cephei variable, although with an effective temperature of about 27,000 K it is...

±0.003 magnitude. For this reason, the star has been ruled out as a Beta Cephei-type variable star. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended...

might comprise a physical binary and an optical companion (such as Beta Cephei) or, in rare cases, a purely optical triple star (such as Gamma Serpentis)...

variable, lying as it does on the overlapping instability strips for Beta Cephei variables and slowly pulsating B-type stars. The star shows at least fourteen...

Grisons. 13131 Palmyra, discovered 1994, and Tadmor, also known as Gamma Cephei Ab, confirmed in 2003, named after Palmyra. 14566 Hōkūleʻa, named 2003 after...

M, Morel T, Ilyin I (April 2009). "New magnetic field measurements of β Cephei stars and slowly pulsating B stars". Astronomische Nachrichten. 330 (4):...

Draconis, Theta Draconis, Zeta Draconis, Upsilon Draconis, 73 Draconis, Gamma Cephei and 23 Cassiopeiae. Consequently, the Chinese name for Eta Draconis itself...

although the actual pole is somewhat offset in the direction of Alpha Cephei; it is more accurate to state that the top two stars of the Northern Cross...

Hubrig, S.; et al. (April 2009), "New magnetic field measurements of β Cephei stars and slowly pulsating B stars", Astronomische Nachrichten, 330 (4):...

Hertzsprung, E. (1913). "Über die räumliche Verteilung der Veränderlichen vom δ Cephei-Typus" [On the spatial distribution of variable [stars] of the δ Cepheid...

One member, HD 74339 (mag. 9.3, spectral type B2/3 II/III), is a beta Cephei variable. "NGC 2539". SIMBAD. Centre de données astronomiques de Strasbourg...

S2CID 119257644. Yüce, Kutluay (2005), "Spectral Analysis of 4 Lacertae and ν Cephei", Baltic Astronomy, 14: 51–82, Bibcode:2005BaltA..14...51Y. Gray, R. O.;...

−60° 43′ 44″ 44.9 ι Piscium F7V 4.06 3.36 23h 39m 57s +05° 37′ 38″ 45.0 γ Cephei A K1IV 2.94 2.24 23h 39m 21s +77° 37′ 56″ 45.0 Gliese 615 K0V 7.36 6.66...

5.0 12.4 281 277+18 −16 [10] R Serpentis 5.2 14.4 356 285+26 −22 [11] T Cephei 5.2 11.3 388 176+13 −12 [12] R Aquarii 5.2 12.4 387 320+31 −26 [13] R Centauri...

of Pi1 Cygni, Alpha Lacertae, 4 Lacertae, Pi2 Cygni, HD 206267, Epsilon Cephei, Beta Lacertae, Sigma Cassiopeiae, Rho Cassiopeiae, Tau Cassiopeiae, AR...

retrieved 4 January 2016 Ritchie, G. W. (1917). "Ritchie's Nova H. IV. 76 Cephei in N.G.C. 6946". Harvard College Observatory Bulletin. 641: 1. Bibcode:1917BHarO...

λ Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae...

2012-01-11 Eggen, O. J. (June 1971), "The ζ Herculis, σ Puppis, ∈ Indi, and η Cephei Groups of Old Disk Population Stars", Publications of the Astronomical Society...

99J Hubrig, S.; et al. (June 2006), "Discovery of magnetic fields in the βCephei star ξ1 CMa and in several slowly pulsating B stars*", Monthly Notices of...

amplitude. This star has unusual variable spectral lines and lies with the β Cephei variable instability strip. However, it is now thought that the variable...

Centauri. Named after Charles Fehrenbach. Herschel's Garnet Star is Mu Cephei, a red supergiant particularly remarkable for its deep red color, first...

stars known in the Milky Way (along with the O-type supergiants Lambda Cephei and Zeta Puppis). Initially it was suggested a supernova explosion of a...

processing BCEP – (celestial object) Beta CEPhei, a class of pulsating variable stars for which Beta Cephei is the archetypal object also BCE BCG – (celestial...

1086/190168. Molenda-Zakowicz, J.; Polubek, G. (December 2005), "New beta Cephei and SPB Stars Discovered in Hipparcos Photometry", Acta Astronomica, 55:...

cippus cippus Fabricius, 1798 Tajuria melastigma de Nicéville, 1887 Charana cepheis de Nicéville, 1894 Rachana jalindra indra Moore, 1883 Creon cleobis cleobis...

retrieved 2021-12-02. Ritchie, G. W. (1917). "Ritchie's Nova H. IV. 76 Cephei in N.G.C. 6946". Harvard College Observatory Bulletin. 641: 1. Bibcode:1917BHarO...

and spectral type also vary. It is classified as a Classical Cepheid (δ Cephei) variable. Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early...

During this period he calculated the mean radius of the variable star Delta Cephei using measurements of its brightness, its colour and the radial velocity...

Its luminosity is varying in a periodic manner similar to that of a Beta Cephei variable. This periodicity has a dozen or more frequencies ranging between...

Size comparison of supergiant and hypergiant stars, including Cygnus OB2 #12, V382 Carinae, Betelgeuse, VV Cephei A, and VY Canis Majoris...

ι Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae...

ψ Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae...

another yellow hypergiant within another massive open cluster, RSGC1 RW Cephei, a K-type red or yellow hypergiant that underwent a "great dimming" event...

Hipparcos satellite, it has been suggested that the runaway star Lambda Cephei may originate from this association, rather than from the adjacent Cepheus...

this star are with Zaofu 造父 (the legendary charioteer, see below) in Zeta Cephei within Cepheus (Chinese astronomy) or in the constellation Scorpius. In...

1.91 4970 FU Tauri b 16.0 800 2375 imaging 2008 456.63 0.05 2838 Gamma Cephei Ab 1.85 903.3 2.05 radial vel. 2003 44.16 1.4 4744 Proper name Tadmor Gamma...

06 magnitude and a period of 0.6096 days, tentatively classified as Beta Cephei variable. The variability was discovered in 1959, and it has been assigned...

"Dynamics of the circumstellar gas in the Herbig Ae stars BF Orionis, SV Cephei, WW Vulpeculae and XY Persei". Astronomy & Astrophysics. 419: 225–240....

7 every 6.22 days. This type of variable is known as a Cepheid after δ Cephei, the first example to be discovered. X Crucis is a population I star and...

Packet Observations with the CHARA Array. II. ω Andromeda, HD 178911, and ξ Cephei", The Astronomical Journal, 148 (3): 8, arXiv:1407.0639, Bibcode:2014AJ...

Paper 241: HR 1884, HD 174103, HD 182563, and HR 8442, with a note on zeta Cephei". The Observatory. 135: 71–95. Bibcode:2015Obs...135...71G. Luck, R. Earle...

October: John Goodricke begins his observations of the variable star Delta Cephei. 1788 – Public dispensary for the poor opened at Merchant Adventurers' Hall...

B-type giant star with a stellar classification of B2.5 III. It is a Beta Cephei variable with an estimated 8.4 times the mass of the Sun and around 7.1...

a radial velocity of −13.5 km/s. This is a Classical Cepheid, or Delta Cephei variable, that ranges in brightness from visual magnitude 6.40 down to 7...

et al. (2015). "The 2003–2004 multisite photometric campaign for the β Cephei and eclipsing star 16 (EN) Lacertae with an appendix on 2 Andromedae, the...

subgiant star with a stellar classification of B2 IV. It is a candidate Beta Cephei variable and is rotating rapidly. Its companion, σ Cassiopeiae B, is a main...

AU. List of star systems within 45–50 light-years Alpha Centauri Gamma Cephei Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation"...

difficult to measure directly. The current mass of Cepheid variables such as δ Cephei can be measured accurately because there are either binaries or pulsating...

Australis Past and future Northern Vega Tianbang Asuusiha Thuban Kochab Errai ι Cephei Alfirk Alderamin Deneb Fawaris Southern β Hydri γ Chamaeleontis I Carinae...

Tadmor Ancient Palmyrene Aramaic and modern Arabic name for Palmyra Gamma Cephei A (Errai) 1.85 903.3 2.05 radial vel. 2003 45.0 1.4 2015 NameExoWorlds Meztli...

planets have been found around evolved K-giant stars including Pollux, Gamma Cephei and Iota Draconis. Doppler surveys around a wide variety of stars indicate...

star system which indicates deceleration by the interstellar medium. VV Cephei Antares Betelgeuse VFTS 352 Rigel WOH G64 "VSX : Detail for HD 302821"....

Extinction Data of 12547 O-Stars to F-Stars Galactic Clusters and Delta-Cephei Stars". Bulletin d'Information du Centre de Donnees Stellaires. 19: 61....

naked eye of an observer far from city lights. V2052 Ophiuchi is a Beta Cephei variable (β Cep) star, varying slightly in brightness from magnitude 5.81...

bow shock-producing red supergiant stars, along with Betelgeuse and Mu Cephei. Unlike the other two, the bow shock is visible in visible light. Its stellar...

retrieved 2012-12-28. Percy, J. R.; Lane, M. C. (May 1977), "Search for Beta Cephei stars. I - Photometric and spectroscopic studies of northern B-type stars"...

Indi) and The Head of Hydrus (Alpha Hydri), Herschel's Garnet Star (Mu Cephei), Barnard's Star, etc. During the 12th century the Byzantines provided their...

inclination. The two stars are both on the main sequence. The primary, a β Cephei pulsator, has a spectral type of B1 and temperature of about 26,000 K, while...

S Persei VX Sagittarii V1804 Sagittarii VY Canis Majoris AH Scorpii MY Cephei PZ Cassiopeiae IRC −30308 NML Cygni IRC +10420 WOH G64 A IRAS 05280−6910...

Uranus () features the capital initial letter of Herschel's surname. Mu Cephei is also known as Herschel's Garnet Star Herschel, a crater on the Moon Herschel...

German astronomer Erich P. Heilmeier for the spectroscopic study of Beta Cephei and other variable stars. Because of the growth of the Santiago metropolis...

The primary, designated component Aa or sometimes just A, displays Beta Cephei-like pulsational behavior. It appears to be a B-type main-sequence star...

second-generation formation that was raised by Ramm et al. (2021). HD 59686 Ab Gamma Cephei Ab Lists of planets Ramm, David J. (2004). A spectroscopic study of detached...

1051/0004-6361:20020525. Hoffmeister, Cuno (1957). "On Two Abnormal Stars of Delta Cephei Type". Astrophysical Journal. 125: 824. Bibcode:1957ApJ...125..824H. doi:10...

pulsations of its surface. The latter, for example, occurs with a Beta Cephei variable star. radio astronomy The subfield of astronomy that studies astronomical...

Delta Pictoris, Latinized from δ Pictoris, is a binary star system in the southern constellation Pictor. It is visible to the naked with a combined apparent...

Some sources also attribute the discovery of another variable star V Cephei or U Cephei to him but same has not been confirmed by the Madras Observatory....

visible to the naked eye, include, besides 10 Lacertae, 12 Lacertae, a Beta Cephei variable with an average magnitude of 5.25, and 16 Lacertae, another Beta...

types F6Ib-II and G1Ib-II. S Crucis is a pulsating variable star of the δ Cephei type, a Classical Cepheid variable. Its mean radius is 37.9 R☉ and that...

parsecs from the Sun; it is an eclipsing binary (with designation V747 Cephei) in which the primary star, of class O5V, has a surface temperature of 45000...

Kilmartin, P. M.; Cottrell, P. L. (January 2004). "Asteroseismology of the β Cephei star ν Eridani - I. Photometric observations and pulsational frequency analysis"...

star. Observations made in 1933 appeared to suggest this could be a Beta Cephei variable, but this was not confirmed by follow-up measurements. The star...

Draconis, Eta Draconis, Theta Draconis, Upsilon Draconis, 73 Draconis, Gamma Cephei and 23 Cassiopeiae. Consequently, the Chinese name for Zeta Draconis itself...

ISSN 0004-637X. Jerzykiewicz, M.; Sterken, C. (1977). "Search for beta Cephei stars south of declination -20 . I. Incidence of light variability among...

Nothodanis schaeffera caesius (Grose-Smith, 1894) Nothodanis schaeffera cepheis (Druce, 1891) Nothodanis schaeffera esme (Grose-Smith, 1894) Paraduba metriodes...

Cakirli, O.; Hoyman, B.; Ozdarcan, O.; Bilir, S. (2025-09-22). "Selected β Cephei pulsators in eclipsing binaries". arXiv:2509.18277 [astro-ph.EP]. Melnik...

variable. Later authors were split on whether it was a symbiotic star or a VV Cephei-type star. The two differ in that the former consists of a red giant and...

magnitude) variability in the brightness of HR 2501 during their search for beta Cephei variable stars in the southern sky. Christoffel Waelkens et al. confirmed...

main sequence (low luminosity) end of the same instability strip as the β Cephei stars would make high-overtone radial pulsations the likely cause. LN And...

κ Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae...

The three systems detected prior to 1994 each have a drawback, with Gamma Cephei Ab being unconfirmed until 2002; while the PSR B1257+12 planets orbit a...

Evidence Supporting Cluster Membership for the Keystone Calibrator Delta Cephei", Astrophysical Journal, 747 (2): 145, arXiv:1201.0993, Bibcode:2012ApJ...

S2CID 14878976. Eggen, O. J. (June 1971), "The ζ Herculis, σ Puppis, ∈ Indi, and η Cephei Groups of Old Disk Population Stars", Publications of the Astronomical Society...

I. & Black, D.C. 2001 “Hipparcos and MAP Studies of the Triple Star Pi Cephei”, ApJ 549, 1145 Gatewood, G., Han, I., Kiewiet de Jonge, J., Reiland, C...

that ranges from 3.49 to 4.3 over a period of 7.177 days. Along with Delta Cephei, Zeta Geminorum and Beta Doradus, it is one of the most prominent naked...

optical spectral scans of U Sagittae : an analysis and comparison with U Cephei", Publications of the Astronomical Society of the Pacific, 97: 138–150,...

Oscillations of α UMa and other red giants, 2001 Asteroseismology of the β Cephei star ν Eridani, 2004 Award of the 3rd Department of Mathematics, Physics...

1902, he discovered the strange behavior of Beta Cephei, which later became the prototype for Beta Cephei variable stars. He played a significant role in...

Crateris (TY Corvi) Corvus 5.19 5.23 0.04 B1.5 V Unknown companion 14 Cephei (LZ Cephei) Cepheus Morris (1985) 4.67 4.71 0.04 O9 III + O9.5 V HZ Canis Majoris...

effective temperature of 27,000 K. ξ1 Canis Majoris is classified as a Beta (β) Cephei variable that ranges from magnitude +4.33 to +4.36 with a period of 5.03...

W26's ejecta to be 403×10−3 M☉, with an uncertainty of ± 94×10−3 M☉. Mu Cephei RSGC1 RSGC1-F01 RSGC1-F02 RSGC1-F13 Applying the Stefan-Boltzmann Law with...

with a stellar classification of B2 IV. It was determined to be a Beta Cephei variable based on observations during 1955 at the Cape Observatory. Tau1...

times more in right ascension than in declination. Delta Ceti is a Beta Cephei variable with a stellar classification of B2 IV. It varies in brightness...

22 April, it was near Beta Cassiopeiae. On 12–14 May, it was near Gamma Cephei. C/2011 L4 continued moving North until 28 May. The comet may have had a...

Scuti variable SX Phoenicis variable Blue-white with early spectra Beta Cephei variable PV Telescopii variable Long Period and Semiregular Mira variable...

Size comparison of Betelgeuse, Mu Cephei, KY Cygni, and V354 Cephei, according to estimates derived in 2005...

Volume of Betelgeuse 1×1036 One cubic terametre 4×1036 Possible volume of μ Cephei (estimates vary) 8×1036 Estimated volume of VY Canis Majoris, a red hypergiant...

interfere with measurements of the primary spectrum. It is a suspected Beta Cephei variable with a period of 0.37968 days and an amplitude of 0.03 magnitude...

Hubrig, S.; et al. (June 2006), "Discovery of magnetic fields in the βCephei star ξ1 CMa and in several slowly pulsating B stars*", Monthly Notices of...

Bibcode:1977MmRAS..84..101B. Jakate, S. M. (1979). "A search for Beta Cephei stars. III - Photometric studies of southern B-type stars". Astronomical...

blue variable (LBV). This is the star Zeta puppis. The red supergiant VV Cephei stars were defined as a class by Bidelman in 1954. In this artist's conception...

presenting as a young B-type main-sequence star. It is classified as a Beta Cephei type variable star and its brightness varies by 0.02 magnitudes with a period...

amplitude. It has a likely period of 0.22132 days and is thought to be a β Cephei variable or slowly pulsating B-type star. Hipparcos photometry shows an...

UBVRI light curves of the prototype Cepheid variable, Delta Cephei...

mass of the Sun and is roughly 15 million years old. Delta Lupi is a Beta Cephei variable star that undergoes periodic pulsations. It has a single period...

; et al. (August 2009), "Imaging and Modeling Rapidly Rotating Stars: α Cephei and α Ophiuchi", The Astrophysical Journal, 701 (1): 209–224, arXiv:0906...

designation, FN Canis Majoris, in 1970. In the past it was classified as a Beta Cephei type variable star with an apparent magnitude that was measured varying...

LGGS J013350.62+303230.3 309,000 3,800 HV 888 302,000 3,442–3,500 M4Ia RW Cephei 300,000 4,400 K2Ia-0 A K-type yellow hypergiant. LGGS J013358.54+303419...

S2CID 119231169. Percy, J. R. (December 1984), "Five suspected Beta Cephei stars revisited", Journal of the Royal Astronomical Society of Canada, 78:...

of Merope varies as a function of time. Merope is classified as a Beta Cephei variable, a type of hot variable star which pulsates regularly due to opacity...

(1947) On the variation of the electronic pressure and the gravity of α Cephei with the phase (1948) Thesis presented at the Faculty of Sciences of the...

Arabic: الراعي, it may also refer to: Alrai, traditional Arabic name of Gamma Cephei, a binary star system in the Cepheus constellation al-Rai, Syria, a town...

Hubrig, S.; et al. (April 2009), "New magnetic field measurements of β Cephei stars and slowly pulsating B stars", Astronomische Nachrichten, 330 (4):...

binary in the constellation Scorpius consisting of a Wolf-Rayet star and a β Cephei variable. It lies 2° west of NGC 6357 on the edge of the Great Rift in the...

The brightest of the five red supergiants is the exceptionally cool MY Cephei. It has a spectral type of M7.5 which is one of the latest spectral types...

as being a confirmed β Cephei variable, but with no explanation of when it was discovered. A 1971 thesis dedicated to β Cephei variables only mentions...

extrasolar planets. The Hermes spectrograph was used to monitor the Star Delta Cephei in the 2010s. The data seemed to suggest a previously unknown stellar companion...

Paper 241: HR 1884, HD 174103, HD 182563, and HR 8442, with a note on zeta Cephei". The Observatory. 135: 71–95. Bibcode:2015Obs...135...71G. Kovtyukh, V...

Hubrig, S.; et al. (April 2009), "New magnetic field measurements of β Cephei stars and slowly pulsating B stars", Astronomische Nachrichten, 330 (4):...

observations suggesting that an extrasolar planet orbits the star Gamma Cephei, although its existence is not confirmed until 2003. Asteroid 3994 Ayashi...

radial velocity of +20 km/s. Eggen (1971) listed it as a member of the η Cephei group of old-disk stars. This is an evolved giant star with a stellar classification...

main-sequence star with a stellar classification of B2V. During a search for Beta Cephei variables in the southern sky, it was initially classed as a very short...

temperature is over 17,000 K, typical of a B-type star. 53 Piscium is a Beta Cephei variable, varying by 0.01 magnitudes just under every two hours. For that...

τ Cassiopeiae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3...

stellar classification of B2.5 IV. Telting and colleagues report it as a Beta Cephei variable with a high degree of confidence as they found regular pulsations...

star is a supergiant. List of nearest supergiants Nearest hypergiant μ Cephei (Garnet Star) 3,060 light-years (940 pc) Nearest carbon star CW Leonis 310...

this star out as a Beta Cephei variable, but the GCVS and the International Variable Star Index classify it as both a Beta Cephei variable and a rotating...

one study, it could be one of the first discovered hybrids between Beta Cephei variables and slowly pulsating B stars. Although not visible to the naked...

oscillating Ap SX Phoenicis Blue-white with early spectra Alpha Cygni Beta Cephei Slowly pulsating B-type PV Telescopii Blue large-amplitude pulsator Long-period...

celestial pole of Mars. The pole is about halfway between Deneb and Alpha Cephei, less than 10° from the former, a bit more than the apparent distance between...

from its birthplace to its current distance. However, its status as a Beta Cephei variable wasn't discovered until a survey of 2000 using Hipparcos data....

1955, and he published that discovery in 1956. It is classified as a Beta Cephei type variable star and its brightness varies from magnitude +4.79 down to...

"Beat of the Drum" (featuring SOFI) Moguai Single March 25 MAU5034 "HR 8938 Cephei" deadmau5 Single April 15 MAU5033 "Raise Your Weapon (Remixes)" deadmau5...

FH Serpentis +4.4 1970 V1229 Aquilae +6.7 1970 V1330 Cygni +7.5 1971 IV Cephei +7.0 1975 V1500 Cygni +1.7 1975 V373 Scuti +6.0 1976 NQ Vulpeculae +6.0...

Telting, J. H.; et al. (2006). "A high-resolution spectroscopy survey of β Cephei pulsations in bright stars". Astronomy and Astrophysics. 452 (3): 945. Bibcode:2006A&A...