14 Aquilae
Star in the constellation Aquila
14 Aquilae is a probable spectroscopic binary [ 10] star system in the equatorial constellation of Aquila . 14 Aquilae is the Flamsteed designation though it also bears the Bayer designation g Aquilae . It is visible to the naked eye as a dim, white-hued star with an apparent visual magnitude of 5.42,[ 2] and it is located at a distance of approximately 500 light-years (150 parsecs ) from Sun. The star is moving closer to the Earth with a heliocentric radial velocity of −39 km/s ,[ 5] and may come as close as 136 light-years in around 3.5 million years.[ 6]
The visible component is an A-type main sequence star with a stellar classification of A1 V.[ 4] It has 3.25[ 3] times the mass of the Sun and about twice the Sun's radius . The projected rotational velocity is relatively low[ 10] at 23 km/s.[ 8] The star is radiating 214[ 7] times the luminosity of the Sun from its photosphere at an effective temperature of 9,908 K.
References
^ a b c d e Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ a b c d Nicolet, B. (1978). "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System". Astronomy and Astrophysics Supplement Series . 34 : 1–49. Bibcode :1978A&AS...34....1N .
^ a b c d e Zorec, J.; Royer, F.; Asplund, Martin; Cassisi, Santi; Ramirez, Ivan; Melendez, Jorge; Bensby, Thomas; Feltzing, Sofia (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy and Astrophysics , 537 : A120, arXiv :1201.2052 , Bibcode :2012A&A...537A.120Z , doi :10.1051/0004-6361/201117691 , S2CID 55586789 .
^ a b Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal , 74 : 375–406, Bibcode :1969AJ.....74..375C , doi :10.1086/110819 .
^ a b Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Carnegie Institute Washington D.C. Publication . Carnegie Institution of Washington . Bibcode :1953GCRV..C......0W .
^ a b Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters , 38 (5): 331, arXiv :1108.4971 , Bibcode :2012AstL...38..331A , doi :10.1134/S1063773712050015 , S2CID 119257644 .
^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics", Astronomy and Astrophysics , 367 (2): 521–524, arXiv :astro-ph/0012289 , Bibcode :2001A&A...367..521P , doi :10.1051/0004-6361:20000451 , S2CID 425754 .
^ a b Royer, F.; Zorec, J.; Gómez, A. E. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics , 463 (2): 671–682, arXiv :astro-ph/0610785 , Bibcode :2007A&A...463..671R , doi :10.1051/0004-6361:20065224 , S2CID 18475298 .
^ "g Aql -- Star" , SIMBAD Astronomical Object Database , Centre de Données astronomiques de Strasbourg , retrieved 2012-07-22 .
^ a b Royer, F.; et al. (February 2014), "Normal A0-A1 stars with low rotational velocities. I. Abundance determination and classification", Astronomy & Astrophysics , 562 : 21, arXiv :1401.2372 , Bibcode :2014A&A...562A..84R , doi :10.1051/0004-6361/201322762 , S2CID 54511685 , A84.
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