Wikipedia

Alpha Cygni variable

(Redirected from Alpha cygni variable)

Alpha Cygni variables are variable stars which exhibit non-radial pulsations, meaning that some portions of the stellar surface are contracting at the same time other parts expand. They are supergiant stars of spectral types B or A. Variations in brightness on the order of 0.1 magnitudes are associated with the pulsations, which often seem irregular, due to beating of multiple pulsation periods. The pulsations typically have periods of several days to several weeks.

The prototype of these stars, Deneb (α Cygni), exhibits fluctuations in brightness between magnitudes +1.21 and +1.29. Small amplitude rapid variations have been known in many early supergiant stars, but they were not formally grouped into a class until the 4th edition of the General Catalogue of Variable Stars was published in 1985. It used the acronym ACYG for Alpha Cygni variable stars.[1] Many luminous blue variables (LBVs) show Alpha Cygni-type variability during their quiescent (hot) phases, but the LBV classification is generally used in these cases.

A large number (32) were discovered by Christoffel Waelkens and colleagues analysing Hipparcos data in a 1998 study.[2]

Pulsations edit

The pulsations of Alpha Cygni Variable stars are not fully understood. They are not confined to a narrow range of temperatures and luminosities in the way that most pulsating stars are. Instead, most luminous A and B supergiants, and possibly also O and F stars, show some type of unpredictable small-scale pulsations. Nonadiabatic strange mode radial pulsations are predicted but only for the most luminous supergiants. Pulsations have also been modelled for less luminous supergiants by assuming they are low mass post-red supergiant stars, but most Alpha Cygni variables do not appear to have passed through the red supergiant stage.[3][4]

The pulsations are likely induced by kappa mechanism, caused by iron opacity variations, with strange modes producing the observed short periods for both radial and non-radial pulsations. Non-adiabatic g-modes may produce longer period variations, but these have not been observed in Alpha Cygni variables.[5]

List edit

Galactic edit

Designation (name) Constellation Discovery Maximum Apparent magnitude (mV)[6] Minimum Apparent magnitude (mV)[6] Period (days) Spectral class Luminosity Comment
CE Cam (HD 21389) Camelopardalis Percy & Welsh (1983)[7] 4m.54 A0Iab 63,000[8]  
CS Cam Camelopardalis Rufener (1982)[9] 4m.259 B9Ia 75,900[10]  
η CMa (Aludra) Canis Major Kazarovets et al. (1999)[11] 2m.38 2m.48 4.70433 B5Ia 105,000[8]  
ο2 CMa Canis Major Waelkens et al. (1998)[2] 2m.98 3m.04 24.44 B3Ia 219,000[12]  
κ Cas Cassiopeia Percy & Welsh (1983)[7] 4m.12 4m.21 2.64690 B1Ia 331,000[12]  
6 Cas Cassiopeia Abt (1957)[13] 5m.34 5m.45 30 B2 Ia+ 200,000[14] Hypergiant
ο2 Cen Centaurus 5m.12 5m.22 46.3 A2Ia 136,000[15]  
ν Cep Cepheus Percy & Welsh (1983)[7] 4m.25 4m.35 A2 Iab 254,000[8]  
DL Cru Crux Waelkens et al. (1998)[2] 6m.24 6m.28 2.8778 B1.5Ia 242,000[16]  
Deneb[4] Cygnus Lee (1910)[17] 1m.21 1m.29 A2 Ia 196,000[18] Prototype
σ Cyg Cygnus Abt (1957)[13] 4m.19 4m.26 120.2 B9 Iab 39,000[19]  
55 Cyg Cygnus Hill et al. (1976)[20] 4m.81 4m.87 B2.5 Ia ~400,000[21]  
3 Gem Gemini Waelkens et al. (1998)[2] 5m.75 13.70 B3 Ia 200,000[22]  
ρ Leo Leo Olsen (1974)[23] 3m.83 3m.9 3.4271 B1Iab 295,000[12]  
β Ori (Rigel)[4] Orion Waelkens et al. (1998)[2] 0m.17 0m.22 B8Ia 279,000[24]

218,000[25]

Brightest member
ε Ori (Alnilam) Orion Cousins (1960)[26] 1m.64 1m.74 B0.5Iabea 275,000[12]

537,000[27]

 
χ2 Ori Orion Waelkens et al. (1998)[2] 4m.68 4m.72 2.8682 B2Ia 446,000[12]  
9 Per Perseus Abt (1957)[13] 5m.15 5m.25 A2 Ia 141,000[28]  

Extragalactic edit

Designation (name) Galaxy Discovery Maximum Apparent magnitude (mV) Minimum Apparent magnitude (mV) Period (days) Spectral class Luminosity Comment
LHA 115-S 18[29] SMC 13m.3 Complex B[e]sg   Possible LBV
HDE 268835[29] LMC 10m.60 10m.68 >100 B8p    
HD 37974[29] LMC 10m.92 11m.00 400 B0.5Ia+    
HD 37836[30] LMC 10m.55 B0Iae LBV candidate

References edit

  1. ^ Kholopov, P. N.; Samus', N. N.; Frolov, M. S.; Goranskij, V. P.; Gorynya, N. A.; Kireeva, N. N.; Kukarkina, N. P.; Kurochkin, N. E.; Medvedeva, G. I.; Perova, N. B. (1996). "VizieR Online Data Catalog: General Catalog of Variable Stars, 4th Ed. (GCVS4) (Kholopov+ 1988)". VizieR On-Line Data Catalog: II/139B. Originally Published in: Moscow: Nauka Publishing House (1985-1988). 2139: 0. Bibcode:1996yCat.2139....0K.
  2. ^ a b c d e f Waelkens, C.; Aerts, C.; Kestens, E.; Grenon, M.; Eyer, L. (1998). "Study of an unbiased sample of B stars observed with Hipparcos: the discovery of a large amount of new slowly pulsating B star". Astronomy and Astrophysics. 330: 215–21. Bibcode:1998A&A...330..215W.
  3. ^ Saio, H.; Georgy, C.; Meynet, G. (2013). "Strange-Mode Instability for Micro-Variations in Luminous Blue Variables". Progress in Physics of the Sun and Stars: A New Era in Helio- and Asteroseismology. Proceedings of a Fujihara Seminar held 25–29 November. Astronomical Society of the Pacific Conference Series. Vol. 479. p. 47. arXiv:1305.4728. Bibcode:2013ASPC..479...47S.
  4. ^ a b c Saio, H.; Georgy, C.; Meynet, G. (2013). "Evolution of blue supergiants and Cygni variables: puzzling CNO surface abundances". Monthly Notices of the Royal Astronomical Society. 433 (2): 1246–1257. arXiv:1305.2474. Bibcode:2013MNRAS.433.1246S. doi:10.1093/mnras/stt796.
  5. ^ Saio, Hideyuki (2011). "Linear analyses for the stability of radial and non-radial oscillations of massive stars". Monthly Notices of the Royal Astronomical Society. 412 (3): 1814–1822. arXiv:1011.4729. Bibcode:2011MNRAS.412.1814S. doi:10.1111/j.1365-2966.2010.18019.x. ISSN 0035-8711. S2CID 118552910.
  6. ^ a b 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: 02025. Bibcode:2009yCat....102025S.
  7. ^ a b c Percy, J. R.; Welch, D. L. (1983). "Photometric variability of B- and A-type supergiants". Publications of the Astronomical Society of the Pacific. 95: 491. Bibcode:1983PASP...95..491P. doi:10.1086/131198. ISSN 0004-6280.
  8. ^ a b c Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), "Masses and luminosities of O- and B-type stars and red supergiants", Astronomische Nachrichten, 331 (4): 349, arXiv:1003.2335, Bibcode:2010AN....331..349H, doi:10.1002/asna.200911355, S2CID 111387483
  9. ^ Rufener, F.; Bartholdi, P. (1982). "List of 333 variable, microvariable or suspected variable stars detected in the Geneva photometry". Astronomy and Astrophysics Supplement Series. 48: 503. Bibcode:1982A&AS...48..503R.
  10. ^ McErlean, N. D.; Lennon, D. J.; Dufton, P. L. (1999). "Galactic B-supergiants: A non-LTE model atmosphere analysis to estimate atmospheric parameters and chemical compositions". Astronomy and Astrophysics. 349: 553. Bibcode:1999A&A...349..553M.
  11. ^ Kazarovets, E. V.; Samus, N. N.; Durlevich, O. V.; Frolov, M. S.; Antipin, S. V.; Kireeva, N. N.; Pastukhova, E. N. (1999). "The 74th Special Name-list of Variable Stars". Information Bulletin on Variable Stars. 4659: 1. Bibcode:1999IBVS.4659....1K.
  12. ^ a b c d e Crowther, P. A.; Lennon, D. J.; Walborn, N. R. (2006). "Physical parameters and wind properties of galactic early B supergiants". Astronomy and Astrophysics. 446 (1): 279–293. arXiv:astro-ph/0509436. Bibcode:2006A&A...446..279C. doi:10.1051/0004-6361:20053685. S2CID 18815761.
  13. ^ a b c Abt, Helmut A. (1957). "The Variability of Supergiants". The Astrophysical Journal. 126: 138. Bibcode:1957ApJ...126..138A. doi:10.1086/146379. ISSN 0004-637X.
  14. ^ Achmad, L.; Lamers, H. J. G. L. M.; Pasquini, L. (1997). "Radiation driven wind models for A, F and G supergiants". Astronomy and Astrophysics. 320: 196. Bibcode:1997A&A...320..196A.
  15. ^ Kaufer, A.; Stahl, O.; Wolf, B.; Gaeng, T.; Gummersbach, C. A.; Kovacs, J.; Mandel, H.; Szeifert, T. (1996). "Long-term spectroscopic monitoring of BA-type supergiants. I. Halpha_ line-profile variability". Astronomy and Astrophysics. 305: 887–901. Bibcode:1996A&A...305..887K.
  16. ^ Lamers, Henny J. G. L. M.; Snow, Theodore P.; Lindholm, Douglas M. (1995). "Terminal Velocities and the Bistability of Stellar Winds". The Astrophysical Journal. 455: 269. Bibcode:1995ApJ...455..269L. doi:10.1086/176575. ISSN 0004-637X.
  17. ^ Lee, O. J. (1910). "Four stars having variable radial velocities". The Astrophysical Journal. 31: 176. Bibcode:1910ApJ....31..176L. doi:10.1086/141741. ISSN 0004-637X.
  18. ^ Schiller, F.; Przybilla, N. (2008). "Quantitative spectroscopy of Deneb". Astronomy & Astrophysics. 479 (3): 849–858. arXiv:0712.0040. Bibcode:2008A&A...479..849S. doi:10.1051/0004-6361:20078590. S2CID 119225384.
  19. ^ Markova, N.; Puls, J. (2008). "Bright OB stars in the Galaxy". Astronomy and Astrophysics. 478 (3): 823–842. arXiv:0711.1110. Bibcode:2008A&A...478..823M. doi:10.1051/0004-6361:20077919. ISSN 0004-6361. S2CID 14510634.
  20. ^ Kholopov, P. N.; Kukarkina, N. P.; Perova, N. B. (1979). "64th Name-List of Variable Stars". Information Bulletin on Variable Stars. 1581: 1. Bibcode:1979IBVS.1581....1K.
  21. ^ Kraus, M.; Haucke, M.; Cidale, L. S.; Venero, R. O. J.; Nickeler, D. H.; Németh, P.; Niemczura, E.; Tomić, S.; Aret, A.; Kubát, J.; Kubátová, B.; Oksala, M. E.; Curé, M.; Kamiński, K.; Dimitrov, W.; Fagas, M.; Polińska, M. (2015). "Interplay between pulsations and mass loss in the blue supergiant 55 Cygnus = HD 198 478". Astronomy & Astrophysics. 581: A75. arXiv:1507.01846. Bibcode:2015A&A...581A..75K. doi:10.1051/0004-6361/201425383. S2CID 55392478.
  22. ^ Kudritzki, R. P.; Puls, J.; Lennon, D. J.; Venn, K. A.; Reetz, J.; Najarro, F.; McCarthy, J. K.; Herrero, A. (1999). "The wind momentum-luminosity relationship of galactic A- and B-supergiants". Astronomy and Astrophysics. 350: 970. arXiv:astro-ph/9910449. Bibcode:1999A&A...350..970K.
  23. ^ Olsen, E. H. (1974). "Variable Stars among the Four-Colour (uvby) Standard Stars". Information Bulletin on Variable Stars. 925: 1. Bibcode:1974IBVS..925....1O.
  24. ^ Chesneau, O.; Kaufer, A.; Stahl, O.; Colvinter, C.; Spang, A.; Dessart, L.; Prinja, R.; Chini, R. (2014). "The variable stellar wind of Rigel probed at high spatial and spectral resolution". Astronomy & Astrophysics. 566: 18. arXiv:1405.0907. Bibcode:2014A&A...566A.125C. doi:10.1051/0004-6361/201322894. S2CID 118404460. A125.
  25. ^ Przybilla, N.; et al. (January 2006). "Quantitative spectroscopy of BA-type supergiants". Astronomy and Astrophysics. 445 (3): 1099–1126. arXiv:astro-ph/0509669. Bibcode:2006A&A...445.1099P. doi:10.1051/0004-6361:20053832. S2CID 118953817.
  26. ^ Cousins, A. W. J. (1960). "New Bright Variable Stars". Monthly Notes of the Astronomical Society of Southern Africa. 19: 56. Bibcode:1960MNSSA..19...56C.
  27. ^ Searle, S. C.; Prinja, R. K.; Massa, D.; Ryans, R. (2008). "Quantitative studies of the optical and UV spectra of Galactic early B supergiants. I. Fundamental parameters". Astronomy and Astrophysics. 481 (3): 777–97. arXiv:0801.4289. Bibcode:2008A&A...481..777S. doi:10.1051/0004-6361:20077125. S2CID 1552752.
  28. ^ Verdugo, E.; Talavera, A.; Gómez De Castro, A. I. (1999). "Understanding A-type supergiants. II. Atmospheric parameters and rotational velocities of Galactic A-type supergiants". Astronomy and Astrophysics. 346: 819. Bibcode:1999A&A...346..819V.
  29. ^ a b c van Genderen, A. M.; Sterken, C. (2002). "Light variations of massive stars (α Cyg variables)". Astronomy and Astrophysics. 386 (3): 926–935. Bibcode:2002A&A...386..926V. doi:10.1051/0004-6361:20020360.
  30. ^ Balona, L A; Handler, G; Chowdhury, S; Ozuyar, D; Engelbrecht, C A; Mirouh, G M; Wade, G A; David-Uraz, A; Cantiello, M (2019-02-27). "Rotational modulation in TESS B stars". Monthly Notices of the Royal Astronomical Society. 485 (3): 3457–3469. arXiv:1902.09470. doi:10.1093/mnras/stz586. ISSN 0035-8711.

Sources edit

  • Samus N.N., Durlevich O.V., et al. Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.)
Retrieved from "https://en.wikipedia.org/w/index.php?title=Alpha_Cygni_variable&oldid=1193634995"