Star in the constellation Eridanus
14 Eridani is astar in theequatorial Eridanus constellation . It has anapparent visual magnitude of 6.143[ 2] radial velocity of around −5 km/s.[ 4] parallax shift ismas [ 1] light years .Proper motion studies indicate that this is anastrometric binary .[ 9] [ 10]
The visible component has astellar classification ofF5 V Fe−0.7 CH−0.5 ,[ 3] spectrum of anF-type main-sequence star with mild underabundances of iron andmethylidyne . It is 1.4[ 6] [ 6] mass of the Sun and 1.5[ 1] Sun's radius . The star is radiating 3.87[ 1] luminosity of the Sun from itsphotosphere at aneffective temperature of 6,719 K.[ 6] X-ray emission .[ 11]
^a b c d e f g h i j 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 atVizieR .^a b c Høg, E.; et al. (2000), "The Tycho-2 catalogue of the 2.5 million brightest stars",Astronomy and Astrophysics ,355 : L27,Bibcode :2000A&A...355L..27H ,doi :10.1888/0333750888/2862 . ^a b Gray, R. O.; et al. (2006), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 pc--The Southern Sample",The Astronomical Journal ,132 (1):161– 170,arXiv :astro-ph/0603770 Bibcode :2006AJ....132..161G ,doi :10.1086/504637 ,S2CID 119476992 . ^a b de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project",Astronomy & Astrophysics ,546 : 14,arXiv :1208.3048 Bibcode :2012A&A...546A..61D ,doi :10.1051/0004-6361/201219219 ,S2CID 59451347 , A61. ^ 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 d e f g David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets",The Astrophysical Journal ,804 (2): 146,arXiv :1501.03154 Bibcode :2015ApJ...804..146D ,doi :10.1088/0004-637X/804/2/146 ,S2CID 33401607 . ^ Casagrande, L.; et al. (June 2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey",Astronomy and Astrophysics ,530 : A138,arXiv :1103.4651 Bibcode :2011A&A...530A.138C ,doi :10.1051/0004-6361/201016276 ,S2CID 56118016 . ^ "14 Eri" .SIMBAD Centre de données astronomiques de Strasbourg . Retrieved2018-01-27 .^ Makarov, V. V.; Kaplan, G. H. (May 2005), "Statistical Constraints for Astrometric Binaries with Nonlinear Motion",The Astronomical Journal ,129 (5):2420– 2427,Bibcode :2005AJ....129.2420M ,doi :10.1086/429590 ^ Frankowski, A.; et al. (March 2007), "Proper-motion binaries in the Hipparcos catalogue. Comparison with radial velocity data",Astronomy and Astrophysics ,464 (1):377– 392,arXiv :astro-ph/0612449 Bibcode :2007A&A...464..377F ,doi :10.1051/0004-6361:20065526 ,S2CID 14010423 . ^ Huensch, M.; et al. (October 1998), "The ROSAT all-sky survey catalogue of optically bright main-sequence stars and subgiant stars",Astronomy and Astrophysics Supplement ,132 (2): 155−171,Bibcode :1998A&AS..132..155H ,doi :10.1051/aas:1998287
