BE Camelopardalis

BE Camelopardalis
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis
Right ascension 03h 49m 31.2819s
Declination +65° 31 33.501
Apparent magnitude (V) 4.47 (4.35 - 4.48[1])
Characteristics
Spectral type M2 II[2]
U−B color index 2.13
B−V color index 1.88
R−I color index 1.42
Variable type Lc[1]
Astrometry
Radial velocity (Rv)3.3 km/s
Proper motion (μ) RA: 2.5 mas/yr
Dec.: 13.98 mas/yr
Parallax (π)3.38 ± 0.63 mas
Distanceapprox. 1,000 ly
(approx. 300 pc)
Details
Temperature3,625[2] K
Other designations
HD 23475, HIP 17884, SAO 12916.
Database references
SIMBADdata
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

BE Camelopardalis (BE Cam) is a star in the constellation Camelopardalis.

BE Camelopardalis is a red M-type bright giant with a mean apparent magnitude of +4.39. It is approximately 965 light years from Earth. It is classified as an irregular variable star and its brightness varies from magnitude +4.35 to +4.48.

References

  1. 1 2 Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S 1. Bibcode:2009yCat....102025S.
  2. 1 2 Levesque, Emily M.; et al. (August 2005), "The Effective Temperature Scale of Galactic Red Supergiants: Cool, but Not As Cool As We Thought", The Astrophysical Journal 628 (2): 973–985, arXiv:astro-ph/0504337, Bibcode:2005ApJ...628..973L, doi:10.1086/430901

External links

This article is issued from Wikipedia - version of the Monday, March 07, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.