Jump to content

R Capricorni

From Wikipedia, the free encyclopedia
The printable version is no longer supported and may have rendering errors. Please update your browser bookmarks and please use the default browser print function instead.
R Capricorni

The visual band light curve of R Capricorni, from AAVSO data[1]
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Capricornus
Right ascension 20h 11m 18.39s[2]
Declination −14° 16′ 04.4″[2]
Apparent magnitude (V) 9.4 to 14.9[3]
Characteristics
Spectral type Cev[2]
Variable type M[3]
Astrometry
Proper motion (μ) RA: 4[2] mas/yr
Dec.: −6[2] mas/yr
Other designations
R Cap, BD−14 5663, GC 28001, SAO 163323, 2MASS J20111833-1416033[2]
Database references
SIMBADdata

R Capricorni (R Cap) is a star in the constellation of Capricornus.[2] It has an apparent visual magnitude which varies between 9.4 and 14.9.[3] A mira variable and ageing red giant, it is in the asymptotic giant branch stage of its lifespan.[4]

R Capricorni is too far from earth for its parallax to be measured effectively; Guandalini and Cristallo calculated the luminosity of Mira variables based on their periods. Using a period of 345.13 days, they calculated the absolute magnitude of R Capricorni to be -4.58.[4]

R Capricorni is losing mass at rate of 2.8*10−6M/year.[5]

References

  1. ^ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  2. ^ a b c d e f g V* R Cap -- Variable Star of Mira Cet type, database entry, SIMBAD. Accessed on line November 9, 2009.
  3. ^ a b c R Cap, database entry, The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars Archived 2017-06-20 at the Wayback Machine, Sternberg Astronomical Institute, Moscow, Russia. Accessed on line November 9, 2009.
  4. ^ a b Guandalini, R.; Cristallo, S. (2013). "Luminosities of carbon-rich asymptotic giant branch stars in the Milky Way". Astronomy & Astrophysics. 555: 7. arXiv:1305.4203. Bibcode:2013A&A...555A.120G. doi:10.1051/0004-6361/201321225. S2CID 54918450. A120.
  5. ^ Uttenthaler, S.; McDonald, I.; Bernhard, K.; Cristallo, S.; Gobrecht, D. (2019), "Interplay between pulsation, mass loss, and third dredge-up: More about Miras with and without technetium", Astronomy & Astrophysics, 622: A120, arXiv:1812.07434, Bibcode:2019A&A...622A.120U, doi:10.1051/0004-6361/201833794, S2CID 119004841