R Cygni

R Cygni is a variable star of the Mira type in the constellation Cygnus, less than 4' from θ Cygni. This is a red giant star on the asymptotic giant branch located around 2,200 light years away. It is an S-type star ranging between spectral types S2.5,9e to S6,9e(Tc).[3]

R Cygni
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension  19h 36m 49.35633s[1]
Declination +50° 11 59.7198[1]
Apparent magnitude (V) 6.1 - 14.4[2]
Characteristics
Spectral type S2.5,9e-S6,9e(Tc)[3]
B−V color index 0.101±0.019[4]
Variable type Mira[2]
Astrometry
Proper motion (μ) RA: −3.158[1] mas/yr
Dec.: −5.755[1] mas/yr
Parallax (π)1.4835 ± 0.0963[1] mas
Distance2,200 ± 100 ly
(670 ± 40 pc)
Details
Radius745[lower-alpha 1] R
Luminosity11,700[5] L
Temperature2,200[6] K
Other designations
R Cyg, BD+49 3064, HD 185456, HIP 31822, SAO 31822, WDS J19368+5012[7]
Database references
SIMBADdata
R Cygni light curve, showing the period-doubling

Stars at this mass range and evolutionary stage are pulsationally unstable, displaying a variation in their light output.[8] R Cygni has a maximum magnitude of 6.1 and a minimum magnitude of 14.4, with a period of 426.45 days.[2] The variation of this star was discovered by English astronomer N. R. Pogson in 1852, and it has a history of recorded brightness measurements stretching back more than a century.[8] R Cygni shows distinct period-doubling, where alternate maxima are of different brightness, hence the real period of pulsation could be considered to be twice that from one maximum to the next.[9]

The Catalog of Components of Double and Multiple Stars lists 10th magnitude BD+49 3065 as a companion to R Cygni, at a separation of 91", and both stars lie at approximately the same distance. The Washington Double Star Catalog additionally lists a 15th magnitude star as a companion at a separation of about 14".[10]

Notes

  1. Applying the Stefan-Boltzmann Law with a nominal solar effective temperature of 5,772 K:
gollark: > God being omnipotent doesn't get bothered by inane syntax, only literal impossibilities. Therefore god could write game engines and shit in Minsky machinesSo an "omnipotent" god can't do logically impossible things, in your øpinion?
gollark: Are deprecated now, yes.
gollark: We have "linter" technology.
gollark: JS *improves* over time, at least.
gollark: You can also use `Array.from`.

References

  1. 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.
  2. Samus', N. N; Kazarovets, E. V; Durlevich, O. V; Kireeva, N. N; Pastukhova, E. N (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085.
  3. BSJ (4 January 2010). "R Cygni". AAVSO Website. American Association of Variable Star Observers. Retrieved 21 January 2014.
  4. 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.
  5. Guandalini, R; Francis, Charles (2010). "Infrared photometry and evolution of mass-losing AGB stars. III. Mass loss rates of MS and S stars". Astronomy and Astrophysics. 513: A4. arXiv:1002.2458. Bibcode:2010A&A...513A...4G. doi:10.1051/0004-6361/200911764.
  6. Ramstedt, S; Schöier, F. L; Olofsson, H (2009). "Circumstellar molecular line emission from S-type AGB stars: Mass-loss rates and SiO abundances". Astronomy and Astrophysics. 499 (2): 515. arXiv:0903.1672. Bibcode:2009A&A...499..515R. doi:10.1051/0004-6361/200911730.
  7. "R Cyg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 30 August 2018.
  8. Kiss, L. L.; Szatmáry, K. (August 2002). "Period-doubling events in the light curve of R Cygni: Evidence for chaotic behaviour". Astronomy and Astrophysics. 390 (2): 585–596. arXiv:astro-ph/0205334. Bibcode:2002A&A...390..585K. doi:10.1051/0004-6361:20020744.
  9. Kiss, L. L; Szatmáry, K (2002). "Period-doubling events in the light curve of R Cygni: Evidence for chaotic behaviour". Astronomy & Astrophysics. 390 (2): 585–596. arXiv:astro-ph/0205334. Bibcode:2002A&A...390..585K. doi:10.1051/0004-6361:20020744.
  10. Mason, Brian D; Wycoff, Gary L; Hartkopf, William I; Douglass, Geoffrey G; Worley, Charles E (2001). "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog". The Astronomical Journal. 122 (6): 3466. Bibcode:2001AJ....122.3466M. doi:10.1086/323920.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.