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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]
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 mas[1]
Distance2,200 ± 100 ly
(670 ± 40 pc)
Details
Mass0.85[4] M
Luminosity11,700[5] L
Surface gravity (log g)−0.50[4] cgs
Temperature2,538[4] K
Metallicity [Fe/H]+0.50[4] dex
Other designations
R Cyg, BD+49 3064, HD 185456, HIP 31822, SAO 31822, WDS J19368+5012[6]
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.[7] 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.[7] 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.[8]

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".[9]

See also edit

References edit

  1. ^ a b c d e 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. ^ a b c 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. S2CID 125853869.
  3. ^ a b BSJ (4 January 2010). "R Cygni". AAVSO Website. American Association of Variable Star Observers. Retrieved 21 January 2014.
  4. ^ a b c d Anders, F.; Khalatyan, A.; Queiroz, A. B. A.; Chiappini, C.; Ardevol, J.; Casamiquela, L.; Figueras, F.; Jimenez-Arranz, O.; Jordi, C.; Monguio, M.; Romero-Gomez, M.; Altamirano, D.; Antoja, T.; Assaad, R.; Cantat-Gaudin, T.; Castro-Ginard, A.; Enke, H.; Girardi, L.; Guiglion, G.; Khan, S.; Luri, X.; Miglio, A.; Minchev, I.; Ramos, P.; Santiago, B. X.; Steinmetz, M. (2022). "VizieR Online Data Catalog: StarHorse2, Gaia EDR3 photo-astrometric distances (Anders+, 2022)". Vizier Online Data Catalog. Bibcode:2022yCat.1354....0A.
  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. S2CID 119193286.
  6. ^ "R Cyg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 30 August 2018.
  7. ^ a b 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. S2CID 17698877.
  8. ^ 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. S2CID 17698877.
  9. ^ 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.

cygni, variable, star, mira, type, constellation, cygnus, less, than, from, cygni, this, giant, star, asymptotic, giant, branch, located, around, light, years, away, type, star, ranging, between, spectral, types, observation, dataepoch, j2000, equinox, j2000co. R Cygni is a variable star of the Mira type in the constellation Cygnus less than 4 from 8 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 dataEpoch J2000 Equinox J2000Constellation CygnusRight ascension 19h 36m 49 35633s 1 Declination 50 11 59 7198 1 Apparent magnitude V 6 1 14 4 2 CharacteristicsSpectral type S2 5 9e S6 9e Tc 3 Variable type Mira 2 AstrometryProper motion m RA 3 158 1 mas yr Dec 5 755 1 mas yrParallax p 1 4835 0 0963 mas 1 Distance2 200 100 ly 670 40 pc DetailsMass0 85 4 M Luminosity11 700 5 L Surface gravity log g 0 50 4 cgsTemperature2 538 4 KMetallicity Fe H 0 50 4 dexOther designationsR Cyg BD 49 3064 HD 185456 HIP 31822 SAO 31822 WDS J19368 5012 6 Database referencesSIMBADdataR Cygni light curve showing the period doublingStars at this mass range and evolutionary stage are pulsationally unstable displaying a variation in their light output 7 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 7 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 8 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 9 See also editList of largest known starsReferences edit a b c d e Brown A G A et al Gaia collaboration August 2018 Gaia Data Release 2 Summary of the contents and survey properties Astronomy amp Astrophysics 616 A1 arXiv 1804 09365 Bibcode 2018A amp A 616A 1G doi 10 1051 0004 6361 201833051 Gaia DR2 record for this source at VizieR a b c 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 S2CID 125853869 a b BSJ 4 January 2010 R Cygni AAVSO Website American Association of Variable Star Observers Retrieved 21 January 2014 a b c d Anders F Khalatyan A Queiroz A B A Chiappini C Ardevol J Casamiquela L Figueras F Jimenez Arranz O Jordi C Monguio M Romero Gomez M Altamirano D Antoja T Assaad R Cantat Gaudin T Castro Ginard A Enke H Girardi L Guiglion G Khan S Luri X Miglio A Minchev I Ramos P Santiago B X Steinmetz M 2022 VizieR Online Data Catalog StarHorse2 Gaia EDR3 photo astrometric distances Anders 2022 Vizier Online Data Catalog Bibcode 2022yCat 1354 0A 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 amp A 513A 4G doi 10 1051 0004 6361 200911764 S2CID 119193286 R Cyg SIMBAD Centre de donnees astronomiques de Strasbourg Retrieved 30 August 2018 a b Kiss L L Szatmary 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 amp A 390 585K doi 10 1051 0004 6361 20020744 S2CID 17698877 Kiss L L Szatmary K 2002 Period doubling events in the light curve of R Cygni Evidence for chaotic behaviour Astronomy amp Astrophysics 390 2 585 596 arXiv astro ph 0205334 Bibcode 2002A amp A 390 585K doi 10 1051 0004 6361 20020744 S2CID 17698877 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 Retrieved from https en wikipedia org w index php title R Cygni amp oldid 1172172712, wikipedia, wiki, book, books, library,

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