Mu Horologii
Star in the constellation Horologium
Mu Horologii (μ Horologii) is a solitary,[ 9] yellow-white hued star in the southern constellation of Horologium . It is faintly visible to the naked eye with an apparent visual magnitude of 5.11.[ 2] Based upon an annual parallax shift of 23.04 mas as seen from Earth,[ 1] it is located about 141.6 light years from the Sun .
This is an evolving F-type star with a stellar classification of F0 III/IV,[ 3] showing mixed traits of a subgiant and a giant star . It is around two billion years old with a projected rotational velocity of 79.2 km/s.[ 5] The star has 1.5[ 6] times the mass of the Sun and is radiating 13[ 7] times the solar luminosity from its photosphere at an effective temperature of 6,898 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 .
^ a b c Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory , 4 (99), Bibcode :1966CoLPL...4...99J .
^ a b Houk, Nancy; Cowley, A. P. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars , vol. 1, Ann Arbor: Dept. of Astronomy, University of Michigan, Bibcode :1975mcts.book.....H .
^ 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.
^ 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 g Ramírez, I.; et al. (September 2012), "Lithium Abundances in nearby FGK Dwarf and Subgiant Stars: Internal Destruction, Galactic Chemical Evolution, and Exoplanets", The Astrophysical Journal , 756 (1): 46, arXiv :1207.0499 , Bibcode :2012ApJ...756...46R , doi :10.1088/0004-637X/756/1/46 , S2CID 119199829 .
^ 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 .
^ "mu. Hor" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2017-04-25 .{{cite web }}
: CS1 maint: postscript (link )
^ 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 .