A-type star in the constellation Eridanus
Tau3 Eridani ,Latinized fromτ3 Eridani , is astar in theconstellation Eridanus . It is visible to the naked eye with anapparent visual magnitude of 4.10.[ 2] Using theparallax method ,[ 1] the distance to this star can be estimated as 88.6 light years . In 2001 it was reported as a candidateVega -like star, meaning it appears to radiate aninfrared excess from an orbitingcircumstellar disk .[ 11] However, this has not been confirmed.[ 12]
This is anA-type star with astellar classification of A3 IV-V.[ 3] Theluminosity class of IV-V indicates the spectrum displays traits intermediate between amain sequence andsubgiant star . It is around 476[ 6] million years old and is spinning rapidly with aprojected rotational velocity of 133 km/s.[ 9] This is creating an equatorial bulge that might be 7% wider than the polar radius.[ 13] Tau3 Eridani has 178%[ 6] of theSun's mass and nearly double theradius of the Sun .[ 7] The star shines with 13.7 times thesolar luminosity from anouter atmosphere at aneffective temperature of 8,251 K.[ 6]
^a b c d e f van Leeuwen, F. (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 ^a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)",Catalogue of Eggen's UBV Data ,SIMBAD ,Bibcode :1986EgUBV........0M . ^a b c Gray, R. O.; et al. (July 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 . ^ Wilson, R. E. (1953), "General Catalogue of Stellar Radial Velocities",Carnegie Institute Washington D.C. Publication , Carnegie Institute of Washington, D.C.,Bibcode :1953GCRV..C......0W . ^ 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. (May 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): 38,arXiv :1501.03154 ,Bibcode :2015ApJ...804..146D ,doi :10.1088/0004-637X/804/2/146 ,S2CID 33401607 , 146. ^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 . ^ McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars",Monthly Notices of the Royal Astronomical Society ,427 (1):343– 57,arXiv :1208.2037 ,Bibcode :2012MNRAS.427..343M ,doi :10.1111/j.1365-2966.2012.21873.x ,S2CID 118665352 . ^a b Royer, F.; et al. (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 . ^ "tau03 Eri" .SIMBAD .Centre de données astronomiques de Strasbourg . Retrieved2016-10-13 .{{cite web }}
: CS1 maint: postscript (link )^ Song, Inseok; et al. (January 2001), "Ages of A-Type Vega-like Stars from uvbyβ Photometry",The Astrophysical Journal ,546 (1):352– 357,arXiv :astro-ph/0010102 ,Bibcode :2001ApJ...546..352S ,doi :10.1086/318269 ,S2CID 18154947 . ^ Gáspár, András; et al. (May 2013), "The Collisional Evolution of Debris Disks",The Astrophysical Journal ,768 (1): 29,arXiv :1211.1415 ,Bibcode :2013ApJ...768...25G ,doi :10.1088/0004-637X/768/1/25 ,S2CID 119295265 , 25. ^ Van Belle, Gerard T. (2012), "Interferometric observations of rapidly rotating stars",The Astronomy and Astrophysics Review ,20 (1): 51,arXiv :1204.2572 ,Bibcode :2012A&ARv..20...51V ,doi :10.1007/s00159-012-0051-2 ,S2CID 119273474 .