HD 76728
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Carina |
| Right ascension | 08h 55m 02.82822s[1] |
| Declination | −60° 38′ 40.5998″[1] |
| Apparent magnitude (V) | +3.84[2] |
| Characteristics | |
| Evolutionary stage | Bright giant |
| Spectral type | B8/9II[3] |
| B−V color index | −0.104±0.006[2] |
| Variable type | Constant[4] |
| Astrometry | |
| Radial velocity (Rv) | +25.0±4.1[2] km/s |
| Proper motion (μ) | RA: −28.18[1] mas/yr Dec.: +41.48[1] mas/yr |
| Parallax (π) | 10.20±0.10 mas [1] |
| Distance | 320 ± 3 ly (98.0 ± 1.0 pc) |
| Absolute magnitude (MV) | −1.12[2] |
| Details | |
| Radius | 4.057[5] R☉ |
| Luminosity | 446[5] L☉ |
| Temperature | 13,180[5] K |
| Other designations | |
| c Car, CD−60°1243, FK5 336, GC 12359, HD 76728, HIP 43783, HR 3571, SAO 250374, CCDM J08550-6039, WDS J08550-6039A[6] | |
| Database references | |
| SIMBAD | data |
HD 76728 is a suspected astrometric binary [7] star system in the constellation Carina. It has the Bayer designation c Carinae; HD 76728 is the identifier from the Henry Draper catalogue . The visible component has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of +3.84.[2] The system is located at a distance of approximately 320 light years from the Sun based on parallax,[1] and it is drifting further away with a radial velocity of around +25 km/s.[2] It is a candidate member of the Volans-Carina Association of co-moving stars.[8]
The visible component is an aging bright giant star with a stellar classification of B8/9II.[3] The spectrum of the star displays metallic lines of magnesium.[9] The Volans-Carina Association to which it belongs has an age of 90 million years.[8] The star has four times the radius of the Sun and is radiating 450 times the Sun's luminosity from its photosphere at an effective temperature of 13,180 K.[5]
References
[edit ]- ^ 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 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; Cowley, A. P. (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts.book.....H
- ^ Adelman, S. J.; et al. (September 2000), "On the Variability of O and B Supergiants", Information Bulletin on Variable Stars, 4946: 1, Bibcode:2000IBVS.4946....1A.
- ^ a b c d Kochukhov, O.; Khalack, V.; Kobzar, O.; Neiner, C.; Paunzen, E.; Labadie-Bartz, J.; David-Uraz, A. (2021年08月10日), "TESS survey of rotational and pulsational variability of mercury-manganese stars", Monthly Notices of the Royal Astronomical Society, 506 (4): 5328–5344, arXiv:2107.09096 , doi:10.1093/mnras/stab2107 , ISSN 0035-8711.
- ^ "HD 76728". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020年01月20日.
- ^ 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 Gagné, Jonathan; et al. (October 2018), "Volans-Carina: A New 90 Myr Old Stellar Association at 85 pc", The Astrophysical Journal, 865 (2): 13, arXiv:1808.04420 , Bibcode:2018ApJ...865..136G, doi:10.3847/1538-4357/aadaed , S2CID 119402144, 136.
- ^ Garrison, R. F.; Gray, R. O. (April 1994), "The Late B-Type Stars: Refined MK Classification, Confrontation With Stromgren Photometry, And The Effects of Rotation", Astronomical Journal, 107: 1556, Bibcode:1994AJ....107.1556G, doi:10.1086/116967.