Binary star system in the constellation Aquila
14 Sagittae is a binary star [ 7] system in the equatorial constellation of Aquila .[ 10] 14 Sagittae is the Flamsteed designation . It appears as a sixth magnitude star, near the lower limit of visibility to the naked eye, having an apparent visual magnitude of 5.89.[ 2] The system is located 660 light years away, as determined from its annual parallax shift of 4.91 mas .[ 1] It is moving closer to the Earth with a heliocentric radial velocity of –22 km/s.[ 4]
This is a single-lined spectroscopic binary with an orbital period of 61.5 days and an eccentricity of 0.49.[ 7] The visible component is a chemically peculiar mercury-manganese star [ 11] with a stellar classification of B9p HgMn .[ 3] It is narrow-lined with a projected rotational velocity of 7 km/s.[ 8] The star is radiating 292[ 6] times the Sun's luminosity from its photosphere at an effective temperature of 13,200 K.[ 3]
References
^ a b c d 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 .
^ a b c d Fernie, J. D. (May 1983), "New UBVRI photometry for 900 supergiants", Astrophysical Journal Supplement Series , 52 : 7– 22, Bibcode :1983ApJS...52....7F , doi :10.1086/190856 .
^ a b c d e Smith, K. C.; Dworetsky, M. M. (July 1993), "Elemental Abundances in Normal Late B-Stars and Hgmn-Stars from Co-Added IUE Spectra - Part One - Iron Peak Elements", Astronomy and Astrophysics , 274 (2): 335, Bibcode :1993A&A...274..335S .
^ a b Wilson, Ralph Elmer (1953), "General Catalogue of Stellar Radial Velocities", Carnegie Institute Washington D.C. Publication , Washington: Carnegie Institution of Washington , Bibcode :1953GCRV..C......0W .
^ a b van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653– 664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600 .
^ a b c 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 c Pourbaix, D.; et al. (2004), "SB9: The Ninth Catalogue of Spectroscopic Binary Orbits", Astronomy & Astrophysics , 424 : 727– 732, arXiv :astro-ph/0406573 , Bibcode :2004A&A...424..727P , doi :10.1051/0004-6361:20041213 , S2CID 119387088 .
^ a b Adelman, S. J.; et al. (June 2017), "Elemental abundance analyses with DAO spectrograms: XL", Astronomische Nachrichten , 338 (5): 584– 597, Bibcode :2017AN....338..584A , doi :10.1002/asna.201613214 .
^ "4 Aql" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved October 27, 2018 .
^ Hoffleit, D.; Warren Jr., W. H. (1991), "The Bright Star Catalogue", New Haven (5th Revised [Preliminary Version] ed.), Astronomical Data Center, NSSDC/ADC, Bibcode :1964cbs..book.....H .
^ Adelman, S. J. (December 1988), "Elemental Abundance Analyses with Coadded DAO Spectrograms - Part Five - the Mercury-Manganese Stars Phi-Herculis 28-HERCULIS and HR:7664", Monthly Notices of the Royal Astronomical Society , 235 (3): 763, Bibcode :1988MNRAS.235..763A , doi :10.1093/mnras/235.3.763 .
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