Binary star in the northern constellation of Boötes
15 Boötis is a binary star [ 2] system in the northern constellation of Boötes ,[ 8] located approximately 260 light years away from the Sun.[ 1] It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.45.[ 2] The system has a relatively high proper motion , traversing the celestial sphere at the rate of 0.166 arc seconds per annum.[ 9] It is moving away from the Earth with a heliocentric radial velocity of +16.8 km/s.[ 4]
The magnitude 5.51[ 2] primary, designated component A, is an aging K-type giant star with a stellar classification of K1 III.[ 3] It is a red clump giant,[ 7] which indicates it is on the horizontal branch and is generating energy through helium fusion at its core . It is around two[ 5] billion years old with 1.5[ 5] times the mass of the Sun and has expanded to 10[ 6] times the Sun's radius . The star is radiating 61[ 4] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,845 K.[ 5]
Its companion, component B, is a magnitude +8.53 star[ 2] was located at an angular separation of 0.80″ along a position angle of 111° from the primary, as of 2015. This is the same separation it had when the system was discovered in 1936.[ 10]
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 e 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 .
^ a b Harlan, E. A.; Taylor, D. C. (March 1970), "MK classification for F- and G-type stars. II", Astronomical Journal , 75 (2): 165– 166, Bibcode :1970AJ.....75..165H , doi :10.1086/110956 .
^ 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 c d e f g Feuillet, Diane K.; et al. (2016), "Determining Ages of APOGEE Giants with Known Distances", The Astrophysical Journal , 817 (1): 40, arXiv :1511.04088 , Bibcode :2016ApJ...817...40F , doi :10.3847/0004-637x/817/1/40 , S2CID 118675933 .
^ a b c Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity", The Astronomical Journal , 135 (1): 209– 231, Bibcode :2008AJ....135..209M , doi :10.1088/0004-6256/135/1/209 , S2CID 121883397
^ a b Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal , 539 (2): 732– 741, arXiv :astro-ph/0003329 , Bibcode :2000ApJ...539..732A , doi :10.1086/309278 , S2CID 16673121 .
^ a b "15 Boo" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved May 7, 2019 .
^ Lépine, Sébastien; Shara, Michael M. (March 2005), "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)", The Astronomical Journal , 129 (3): 1483– 1522, arXiv :astro-ph/0412070 , Bibcode :2005AJ....129.1483L , doi :10.1086/427854 , S2CID 2603568 .
^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog" , The Astronomical Journal , 122 (6): 3466, Bibcode :2001AJ....122.3466M , doi :10.1086/323920 , retrieved 2015-07-22 .