Star in the constellation Centaurus
HD 111968 , also known by the Bayer designation n Centauri , is a single[ 8] star in the southern constellation of Centaurus . It is a white-hued star that is faintly visible to the naked eye with an apparent visual magnitude of +4.25.[ 2] The star is located at a distance of approximately 149 light years from the Sun based on parallax .[ 1] The radial velocity of the star is poorly constrained, with an estimated value of 2.5 km/s.[ 2]
This is classified as an A-type star but there has been disagreement about the luminosity class . A. de Vaucouleurs in 1957 found a class of III, suggesting this is an evolved giant star .[ 9] O. J. Eggen gave a class of V in 1962,[ 10] as did R. O. Gray and R. F. Garrison in 1989,[ 4] indicating this is a main sequence star. In 1979, N. Houk found a class of IV,[ 3] meaning this is a subgiant star .
HD 111968 is a young star, some 400 million years old, with 1.6 times the mass of the Sun.[ 6] It is spinning with a projected rotational velocity of 92 km/s.[ 5] The star is radiating 34[ 2] times the luminosity of the Sun from its photosphere at an effective temperature of 7,835 K.[ 6]
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 . Vizier catalog entry
^ a b c d e f 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 Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars , vol. 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode :1982mcts.book.....H .
^ a b Gray, R. O.; Garrison, R. F. (1989), "The Late A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation", The Astrophysical Journal Supplement Series , 70 : 623, Bibcode :1989ApJS...70..623G , doi :10.1086/191349 .
^ a b c Ammler-von Eiff, Matthias; Reiners, Ansgar (June 2012), "New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?", Astronomy & Astrophysics , 542 : A116, arXiv :1204.2459 , Bibcode :2012A&A...542A.116A , doi :10.1051/0004-6361/201118724 , S2CID 53666672 .
^ 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 .
^ "n Cen" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-10-01 .
^ 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 .
^ de Vaucouleurs, A. (1957). "Spectral types and luminosities of B, A and F southern stars" . Monthly Notices of the Royal Astronomical Society . 117 (4): 449. Bibcode :1957MNRAS.117..449D . doi :10.1093/mnras/117.4.449 .
^ Eggen, O. J. (1962), "Space-velocity vectors for 3483 stars with proper motion and radial velocity", Royal Observatory Bulletin , 51 : 79, Bibcode :1962RGOB...51...79E .