R Equulei

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R Equulei
REquLightCurve.png
The visual band light curve of R Equulei, from AAVSO data [1]
Observation data
Epoch J2000       Equinox J2000
Constellation Equuleus
Right ascension 21h 13m 11.49118s [2]
Declination 12° 48′ 06.1620″ [2]
Apparent magnitude  (V)8.7 - 15.0 [3]
Characteristics
Spectral type M3e - M4e [3]
B−V color index +1.41 [4]
Variable type Mira [3]
Astrometry
Radial velocity (Rv)−54±5 [5]  km/s
Proper motion (μ)RA: −2.713 [2]   mas/yr
Dec.: −11.232 [2]   mas/yr
Parallax (π)0.4329 ± 0.0437  mas [2]
Distance approx. 7,500  ly
(approx. 2,300  pc)
Details
Mass 3.42 [6]   M☉
Luminosity 33,791 [7]   L☉
Surface gravity (log g)−0.007 [6]   cgs
Temperature 3,395 [6]   K
Metallicity [Fe/H]−0.13 [6]   dex
Other designations
R Equ, BD+12°4573a, HD  202051, PPM  139768 [8]
Database references
SIMBAD data

R Equulei is a class M Mira variable star in the constellation Equuleus. Its brightness varies between a minimum magnitude of 15.0 to a maximum of 8.7 with an average period of 261 days. [3]

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References

  1. ↑ "Download Data". aavso.org. AAVSO. Retrieved 1 October 2021.
  2. 1 2 3 4 5 Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics . 649: A1. arXiv: 2012.01533 . Bibcode:2021A&A...649A...1G. doi: 10.1051/0004-6361/202039657 . S2CID   227254300. (Erratum:  doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  3. 1 2 3 4 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: B/gcvs, Bibcode:2009yCat....102025S.
  4. ↑ Zacharias, N.; et al. (2012), "The fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)", VizieR On-line Data Catalog, 1322 (2): 44, arXiv: 1212.6182 , Bibcode:2012yCat.1322....0Z, doi:10.1088/0004-6256/145/2/44, S2CID   119299381.
  5. ↑ Wilson, Ralph Elmer (1953), "General catalogue of stellar radial velocities", Washington, Carnegie Institution of Washington: 0, Bibcode:1953GCRV..C......0W.
  6. 1 2 3 4 Anders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019), "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18", Astronomy and Astrophysics, 628: A94, arXiv: 1904.11302 , Bibcode:2019A&A...628A..94A, doi:10.1051/0004-6361/201935765, S2CID   131780028.
  7. ↑ 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.
  8. ↑ "V* R Equ". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2012-09-17.


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