BU Canis Minoris
BU Canis Minoris is a binary star[6] system in the equatorial constellation of Canis Minor. It has the Henry Draper Catalogue designation of HD 65241, while BU Canis Minoris is its variable star designation. The system is a challenge to view with the naked eye, having a peak apparent visual magnitude of 6.42.[2] It is located at a distance of approximately 700 light years from the Sun based on parallax,[1] and is drifting further away with a radial velocity of about +34 km/s.[2]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Canis Minor |
Right ascension | 07h 58m 05.89734s[1] |
Declination | 07° 12′ 48.7030″[1] |
Apparent magnitude (V) | 6.42[2] |
Characteristics | |
Spectral type | A0V[3] |
B−V color index | −0.031±0.008[2] |
Astrometry | |
Radial velocity (Rv) | +34.0±6.5[2] km/s |
Proper motion (μ) | RA: −9.407[1] mas/yr Dec.: −11.835[1] mas/yr |
Parallax (π) | 4.0663 ± 0.0568[1] mas |
Distance | 800 ± 10 ly (246 ± 3 pc) |
Absolute magnitude (MV) | −0.38[2] |
Details | |
Radius | 2.0[4] R☉ |
Luminosity | 158.70[2] L☉ |
Temperature | 10829±797[5] K |
Rotational velocity (v sin i) | ~70[6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
This pair is a double-lined spectroscopic binary system[6] that forms an Algol-like eclipsing binary. The brightness of the system decreases from 6.44 down to 6.53 during the primary eclipse.[8] It has a stellar classification of A0V,[3] which matches an A-type main-sequence star that is generating energy through hydrogen fusion at its core.
References
- 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. Gaia DR2 record for this source at VizieR.
- 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.
- Cowley, A.; Cowley, C.; Jaschek, M.; Jaschek, C. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819
- Pasinetti Fracassini, L. E.; et al. (2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy & Astrophysics (Third ed.), 367 (2): 521–24, arXiv:astro-ph/0012289, Bibcode:2001A&A...367..521P, doi:10.1051/0004-6361:20000451, S2CID 425754.
- Paunzen, E.; et al. (October 2006), "An empirical temperature calibration for the Δ a photometric system. II. The A-type and mid F-type stars", Astronomy and Astrophysics, 458 (1): 293–296, arXiv:astro-ph/0607567, Bibcode:2006A&A...458..293P, doi:10.1051/0004-6361:20064889, S2CID 18219735.
- Dworetsky, Michael M. (November 1974), "Rotational Velocities of a0 Stars", Astrophysical Journal Supplement, 28: 101, Bibcode:1974ApJS...28..101D, doi:10.1086/190312.
- "BU CMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-11.
- Samus, N. N.; et al. (2017), "General Catalogue of Variable Stars", Astronomy Reports, 5.1, 61 (1): 80–88, Bibcode:2017ARep...61...80S, doi:10.1134/S1063772917010085, S2CID 125853869.