Misplaced Pages

HD 81799

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
(Redirected from G Hydrae) Star and suspected binary system in the constellation Hydra
HD 81799
Observation data
Epoch J2000      Equinox J2000
Constellation Hydra
Right ascension 09 27 18.43258
Declination −22° 20′ 37.4967″
Apparent magnitude (V) 4.69
Characteristics
Spectral type K2+ IIIb
B−V color index 1.154
Astrometry
Radial velocity (Rv)29.05±0.28 km/s
Proper motion (μ) RA: +160.160 mas/yr
Dec.: −173.131 mas/yr
Parallax (π)19.8887 ± 0.3128 mas
Distance164 ± 3 ly
(50.3 ± 0.8 pc)
Absolute magnitude (MV)1.32
Details
Radius10.6 R
Luminosity41.97 L
Surface gravity (log g)2.43 cgs
Temperature4,490 K
Metallicity −0.01 dex
Other designations
G Hya, BD−21° 2802, HD 81799, HIP 46371, HR 3749, SAO 177469, LTT 3479
Database references
SIMBADdata

HD 81799 (G Hydrae) is a suspected astrometric binary star system in the equatorial constellation of Hydra. It is visible to the naked eye with an apparent visual magnitude of 4.69. The distance to this system, as determined from an annual parallax shift of 19.9 mas, is 164 light years. It is moving further away from the Earth with a heliocentric radial velocity of 29 km/s. The system has a relatively high rate of proper motion, traversing the celestial sphere at the rate of 233±19 mas/yr along a position angle of 136°.

The stellar classification of the visible component is K2+ IIIb, which matches an evolved K-type giant star. It is a red clump star, which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. The interferometry-measured angular diameter of the primary, after correcting for limb darkening, is 1.96±0.03 mas, which, at its estimated distance, equates to a physical radius of about 10.6 times the radius of the Sun. It is radiating 42 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,490 K.

The system is a likely (99.4% chance) source of the X-ray emission coming from these coordinates.

References

  1. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051.
  2. ^ Soubiran, C.; Le Campion, J.-F.; Cayrel de Strobel, G.; Caillo, A. (June 2010), "The PASTEL catalogue of stellar parameters", Astronomy and Astrophysics, 515: A111, arXiv:1004.1069, Bibcode:2010A&A...515A.111S, doi:10.1051/0004-6361/201014247, S2CID 118362423.
  3. ^ Keenan, P.; McNeil, R. (October 1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245–266, Bibcode:1989ApJS...71..245K, doi:10.1086/191373
  4. ^ 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.
  5. ^ 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.
  6. ^ Lang, Kenneth R. (2006), Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by:
    2 R = ( 10 3 50.3 1.96 )   AU 0.0046491   AU / R 21.2 R {\displaystyle {\begin{aligned}2\cdot R_{*}&={\frac {(10^{-3}\cdot 50.3\cdot 1.96)\ {\text{AU}}}{0.0046491\ {\text{AU}}/R_{\bigodot }}}\\&\approx 21.2\cdot R_{\bigodot }\end{aligned}}}
  7. "HD 81799". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-24.
  8. Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
  9. Wroblewski, H.; Torres, C. (March 1998), "New proper motion determination of Luyten catalogue stars (LTT) with declination between -5° and -30° and right ascension between 0h and 13h 30m", Astronomy and Astrophysics Supplement, 128: 457–458, Bibcode:1998A&AS..128..457W, doi:10.1051/aas:1998157.
  10. Richichi, A.; et al. (February 2005), "CHARM2: An updated Catalog of High Angular Resolution Measurements", Astronomy and Astrophysics, 431 (2): 773–777, Bibcode:2005A&A...431..773R, doi:10.1051/0004-6361:20042039
  11. Haakonsen, Christian Bernt; Rutledge, Robert E. (September 2009), "XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources", The Astrophysical Journal Supplement, 184 (1): 138–151, arXiv:0910.3229, Bibcode:2009ApJS..184..138H, doi:10.1088/0067-0049/184/1/138, S2CID 119267456.
Constellation of Hydra
Stars
Bayer
Flamsteed
Variable
HR
HD
Gliese
Other
Star clusters
Open
Globular
Nebulae
Planetary
Galaxies
Messier
NGC
Other
Galaxy clusters
Abell
Other
Astronomical events
Categories: