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BC Canis Minoris

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Star in the constellation Canis Minor
BC Canis Minoris

A visual band light curve for BC Canis Minoris, plotted from data presented by Tabur et al. (2009)
Observation data
Epoch J2000      Equinox J2000
Constellation Canis Minor
Right ascension 07 52 07.19000
Declination 03° 16′ 38.4465″
Apparent magnitude (V) 6.30 (6.14 to 6.42)
Characteristics
Evolutionary stage AGB
Spectral type M4/5III
B−V color index 1.464±0.015
Variable type SRb
Astrometry
Radial velocity (Rv)−66.91±0.24 km/s
Proper motion (μ) RA: +49.415 mas/yr
Dec.: −78.835 mas/yr
Parallax (π)6.2916 ± 0.1748 mas
Distance520 ± 10 ly
(159 ± 4 pc)
Absolute magnitude (MV)0.36
Details
Radius60.4+7.6
−10.3 R
Luminosity496.7±15.9 L
Temperature3,507+344
−201 K
Other designations
BC CMi, BD+03°1824, HD 64052, HIP 38406, HR 3061, SAO 116054
Database references
SIMBADdata

BC Canis Minoris is a variable star in the equatorial constellation of Canis Minor. It has a reddish hue and is just barely visible to the naked eye with an apparent visual magnitude that fluctuates around 6.30. The distance to this object is approximately 520 light years based on parallax, but it is drifting closer with a radial velocity of −67 km/s.

In 1962, Alan William James Cousins announced that HR 3061 is a variable star. It was given its variable star designation, BC Canis Minoris, in 1975. It is an aging red giant star currently on the asymptotic giant branch with a stellar classification of M4/5III. It is a semi-regular variable of subtype SRb with measured pulsation periods of 27.7, 143.3 and 208.3 days, and an average visual magnitude of 6.30. With the supply of hydrogen at its core exhausted, it has cooled and expanded off the main sequence and now has around 60 times the girth of the Sun. On average, the star is radiating about 497 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,507 K.

References

  1. Tabur, V.; Bedding, T. R.; Kiss, L. L.; Moon, T. T.; Szeidl, B.; Kjeldsen, H. (December 2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society. 400 (4): 1945–1961. arXiv:0908.3228. Bibcode:2009MNRAS.400.1945T. doi:10.1111/j.1365-2966.2009.15588.x.
  2. ^ 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.
  3. ^ 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.
  4. ^ 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.
  5. ^ Eggen, Olin J. (July 1992). "Asymptotic giant branch stars near the sun". Astronomical Journal. 104 (1): 275–313. Bibcode:1992AJ....104..275E. doi:10.1086/116239.
  6. ^ Houk, N.; Swift, C. (1999). "Michigan catalogue of two-dimensional spectral types for the HD Stars". Michigan Spectral Survey. 5. Bibcode:1999MSS...C05....0H.
  7. "BC CMi". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-12-13.
  8. Cousins, A. W. J. (1963). "Photometric Data for Stars in the Equatorial Zone (Fourth List)". Monthly Notes of the Astron. Soc. Southern Africa. 22: 58–62. Bibcode:1963MNSSA..22...58C. Retrieved 9 December 2024.
  9. Kukarkin, B. V.; Kholopov, P. N.; Kukarkina, N. P.; Perova, N. B. (January 1975). "60th Name-List of Variable Stars" (PDF). Information Bulletin on Variable Stars. 961: 1–15. Bibcode:1975IBVS..961....1K. Retrieved 9 December 2024.
  10. Tabur, V.; Bedding, T. R. (2009). "Long-term photometry and periods for 261 nearby pulsating M giants". Monthly Notices of the Royal Astronomical Society. 400 (4): 1945–61. arXiv:0908.3228. Bibcode:2009MNRAS.400.1945T. doi:10.1111/j.1365-2966.2009.15588.x. S2CID 15358380.
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