V416 Возничего

V416 Возничего
Звезда
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Наблюдательные данные
(Эпоха J2000.0)
Прямое восхождение 5ч 13м 13,33с[1]
Склонение +40° 11′ 36,71″[1]
Расстояние 1433,8973 ± 106,9152 пк[1]
Видимая звёздная величина (V) 7,38[2]
Созвездие Возничий
Астрометрия
Лучевая скорость (Rv) 7 ± 3 км/с[3]
Собственное движение
 • прямое восхождение 0,527 ± 0,083 mas/год[1]
 • склонение −5,192 ± 0,065 mas/год[1]
Параллакс (π) 0,6974 ± 0,052 mas[1]
Спектральные характеристики
Спектральный класс OB[4]
Показатель цвета
 • B−V −0,02
 • U−B −0,68
Коды в каталогах

HD 33604, ALS 8235, CEL 565, GCRV 3086, GSC 02900-00112, HIC 24326, HIP 24326, 2MASS J05131333+4011368, NSV 1871, PPM 47857, SAO 40133, TD1 4176, UBV 4972, UBV M 10699, UCAC2 45793531, uvby98 100033604, [JE82] 155, AG+40 599, BD+40 1213, TYC 2900-112-1, Gaia DR1 188925097273253376, WEB 4718, Gaia DR2 188925101571287168, V416 Aur, EM* MWC 103, GEN# +1.00033604, Hilt 439, LF 7 +40 441, LS V +40 36, MCW 289, MSX5C G166.9465+00.6744, SKY# 8213, [KW97] 21-39, AAVSO 0506+40 и TIC 187689999

Информация в базах данных
SIMBAD HD 33604
Логотип Викиданных Информация в Викиданных ?

V416 Возничего (лат. V416 Aurigae), HD 33604 — двойная звезда в созвездии Возничего на расстоянии приблизительно 4677 световых лет (около 1434 парсеков) от Солнца. Видимая звёздная величина звезды — от +7,48m до +7,23m[5].

Характеристики

Первый компонент — бело-голубая эруптивная переменная Be-звезда типа Гаммы Кассиопеи (GCAS:) спектрального класса B2V:pe[5][6][7][8][9], или B2,5IV[10][11], или B3[12][13]. Масса — около 6,348 солнечных, радиус — около 13,79 солнечных[14]. Эффективная температура — около 9296 K[15].

Второй компонент — коричневый карлик. Масса — около 19,51 юпитерианских[14]. Удалён на 2,769 а.е.[14].

Примечания

  1. ↑ 1 2 3 4 5 6 Gaia Data Release 2 (англ.) / Data Processing and Analysis Consortium, European Space Agency — 2018.
  2. ↑ SIMBAD Astronomical Database
  3. ↑ Gontcharov G. A. Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system (англ.) // Astronomy Letters / R. Sunyaev — Nauka, Springer Science+Business Media, 2006. — Vol. 32, Iss. 11. — P. 759–771. — ISSN 1063-7737; 1562-6873; 0320-0108; 0360-0327 — doi:10.1134/S1063773706110065 — arXiv:1606.08053
  4. ↑ Hardorp J., Theile I., Voigt H. H. Luminous Stars in the Northern Milky Way — 1965. — Т. 5. — С. 0.
  5. ↑ 1 2 V416 Aur Архивная копия от 22 января 2021 на Wayback Machine, database entry, Combined General Catalog of Variable Stars (GCVS5.1, 2017 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Архивная копия от 1 июля 2015 на Wayback Machine Accessed online 2021-01-17.
  6. ↑ Xu Y., Bian S. B., Reid M. J., Li J. J., Zhang B., Yan Q. Z., Dame T. M., Menten K. M., He Z. H., Liao S. L. et al. A comparison of the local spiral structure from Gaia DR2 and VLBI maser parallaxes (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2018. — Vol. 616. — 4 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201833407 — arXiv:1807.00315
  7. ↑ Labadie-Bartz J., Pepper J., McSwain M. V., Bjorkman J. E., Bjorkman K. S., Stevens D. J., James D. J., Kuhn R. B., Siverd R. J., Beatty T. G. Photometric Variability of the Be Star Population (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2017. — Vol. 153, Iss. 6. — 21 p. — ISSN 0004-6256; 1538-3881 — doi:10.3847/1538-3881/AA6396 — arXiv:1609.08449
  8. ↑ Chen P. S., Liu J. Y., Shan H. G. A new approach to the infrared photometric study of Be stars (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2016. — Vol. 463, Iss. 2. — P. 1162–1172. — ISSN 0035-8711; 1365-2966 — doi:10.1093/MNRAS/STW1757
  9. ↑ Reed B. C. New Estimates of the Solar-Neighborhood Massive Star Birthrate and the Galactic Supernova Rate (англ.) // The Astronomical Journal / J. G. III, E. Vishniac — New York City: IOP Publishing, AAS, University of Chicago Press, AIP, 2005. — Vol. 130, Iss. 4. — P. 1652—1657. — ISSN 0004-6256; 1538-3881 — doi:10.1086/444474 — arXiv:astro-ph/0506708
  10. ↑ Clark J. S., Steele I. A. A representative sample of Be stars. II. K band spectroscopy (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2000. — Vol. 141. — P. 65–77. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/AAS:2000310
  11. ↑ Steele I. A., Negueruela I., Clark J. S. A representative sample of Be stars. I. Sample selection, spectral classification and rotational velocities (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 1999. — Vol. 137. — P. 147–156. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/AAS:1999478 — arXiv:astro-ph/9903458
  12. ↑ Cannon A. J., Pickering E. C. VizieR Online Data Catalog: Henry Draper Catalogue and Extension, published in Ann. Harvard Obs. 91-100 (1918-1925) (англ.) // Annals of the Astronomical Observatory of Harvard College — 1918. — Vol. 91-100.
  13. ↑ Roeser S., Bastian U. PPM (Positions and Proper Motions) North Star Catalogue (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 1988. — Vol. 74. — P. 449. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846
  14. ↑ 1 2 3 Kervella P., Arenou F., Mignard F., Thévenin F. Stellar and substellar companions of nearby stars from Gaia DR2. Binarity from proper motion anomaly (англ.) // Astronomy and Astrophysics / T. Forveille — EDP Sciences, 2019. — Vol. 623. — P. 72–72. — 23 p. — ISSN 0004-6361; 0365-0138; 1432-0746; 1286-4846 — doi:10.1051/0004-6361/201834371 — arXiv:1811.08902
  15. ↑ McDonald I., Zijlstra A. A., Boyer M. L. Fundamental parameters and infrared excesses of Hipparcos stars (англ.) // Monthly Notices of the Royal Astronomical Society / D. Flower — OUP, 2012. — Vol. 427, Iss. 1. — P. 343—357. — 15 p. — ISSN 0035-8711; 1365-2966 — doi:10.1111/J.1365-2966.2012.21873.X — arXiv:1208.2037

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