Star in the constellation Taurus
Delta2 Tauri (δ2 Tauri ) is a solitary,[ 10] white-hued star in the zodiac constellation of Taurus . Based upon an annual parallax shift of 20.21 mas as seen from Earth,[ 1] it is located roughly 161 light years distant from the Sun . It is separated from δ1 Tauri by 0.3° on the sky[ 11] and is faintly visible to the naked eye with an apparent visual magnitude of +4.80.[ 2] The star is considered a member of the Hyades cluster .[ 12]
At the estimated age of 449 million years,[ 6] this is an A-type main-sequence star with a stellar classification of A2 Vs,[ 3] where the 's' suffix indicates narrow (sharp) absorption lines . It has 1.8[ 6] times the mass of the Sun and about 1.8[ 7] times the Sun's radius . The star is radiating 27[ 8] times the Sun's luminosity from its photosphere at an effective temperature of 7,997 K.[ 4]
δ2 Tauri is a source of X-ray emission with a luminosity of 101.1× 1020 W . Since A-type stars are not normally a source of X-rays, this emission may be coming from an unknown companion or from a line of sight source.[ 13]
References
^ 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 Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory , 4 (99): 99, Bibcode :1966CoLPL...4...99J .
^ a b Paunzen, E.; et al. (July 2001), "A spectroscopic survey for λ Bootis stars. II. The observational data", Astronomy and Astrophysics , 373 (2): 625– 632, Bibcode :2001A&A...373..625P , doi :10.1051/0004-6361:20010630 .
^ a b c d e f Gebran, M.; et al. (May 2016), "A new method for the inversion of atmospheric parameters of A/Am stars", Astronomy & Astrophysics , 589 : 10, arXiv :1603.01146 , Bibcode :2016A&A...589A..83G , doi :10.1051/0004-6361/201528052 , S2CID 118549566 , A83.
^ Eggen, Olin J. (July 1998), "The Age Range of Hyades Stars", The Astronomical Journal , 116 (1): 284– 292, Bibcode :1998AJ....116..284E , doi :10.1086/300413 .
^ a b c d 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 .
^ a b Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics , 367 (2) (Third ed.): 521– 524, arXiv :astro-ph/0012289 , Bibcode :2001A&A...367..521P , doi :10.1051/0004-6361:20000451 , S2CID 425754 .
^ a b Zorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics , 537 : A120, arXiv :1201.2052 , Bibcode :2012A&A...537A.120Z , doi :10.1051/0004-6361/201117691 , S2CID 55586789 .
^ "del02 Tau" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-08-07 .
^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869– 879, arXiv :0806.2878 , Bibcode :2008MNRAS.389..869E , doi :10.1111/j.1365-2966.2008.13596.x , S2CID 14878976 .
^ O'Meara, Stephen James (2016), Deep-Sky Companions: The Caldwell Objects , Cambridge University Press , p. 195, ISBN 978-1107083974 .
^ Gebran, M.; Vick, M.; Monier, R.; Fossati, L. (November 2010), "Chemical composition of A and F dwarfs members of the Hyades open cluster", Astronomy and Astrophysics , 523 : 13, arXiv :1006.5284 , Bibcode :2010A&A...523A..71G , doi :10.1051/0004-6361/200913273 , S2CID 7164596 , A71.
^ Schröder, C.; Schmitt, J. H. M. M. (November 2007), "X-ray emission from A-type stars", Astronomy and Astrophysics , 475 (2): 677– 684, Bibcode :2007A&A...475..677S , doi :10.1051/0004-6361:20077429 .