Theta1 Crucis
Spectroscopic binary star system in the constellation Crux
Theta1 Crucis (θ1 Cru, Theta 1 Crucis) is a spectroscopic binary star system in the southern constellation of Crux . It is visible to the naked eye with an apparent visual magnitude of 4.30m .[ 2] The distance to this star, as determined using parallax measurements,[ 1] is around 235 light years .
The pair orbit each other closely with a period of 24.5 days and an eccentricity of 0.61.[ 6] The primary component is an Am star , which is a chemically peculiar A-type star that shows anomalous variations in absorption lines of certain elements.[ 10] It has a stellar classification of A3(m)A8-A8.[ 3] With a mass 157% times that of the Sun,[ 7] it radiates 81[ 8] times the Sun's luminosity from its outer atmosphere at an effective temperature of 7341 K.[ 7] Unusually for a fully radiative A-type star, X-ray emissions have been detected, which may instead be coming from the orbiting companion.[ 11]
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^ a b c d Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data , SIMBAD , Bibcode :1986EgUBV........0M .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 Houk, N.; Cowley, A. P. (1975), University of Michigan Catalogue of two-dimensional spectral types for the HD stars , vol. 1, Bibcode :1975mcts.book.....H .
^ 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 .
^ 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 Pourbaix, D.; Tokovinin, A. A.; Batten, A. H.; Fekel, F. C.; Hartkopf, W. I.; et al. (2004), "SB9 : The ninth catalogue of spectroscopic binary orbits", Astronomy & Astrophysics , 424 (2): 727–732, arXiv :astro-ph/0406573 , Bibcode :2004A&A...424..727P , doi :10.1051/0004-6361:20041213 , S2CID 119387088 .
^ a b c d e f 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 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 .
^ "tet01 Cru" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2016-10-06 .{{cite web }}
: CS1 maint: postscript (link )
^ Renson, P.; Manfroid, J. (May 2009), "Catalogue of Ap, HgMn and Am stars" , Astronomy and Astrophysics , 498 (3): 961–966, Bibcode :2009A&A...498..961R , doi :10.1051/0004-6361/200810788 .
^ 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 .