Tham khảo Sao_siêu_khổng_lồ_vàng

  1. ↑ Wallenquist, Aå (1929). “An attempt to determine the mean masses of the stars in the globular cluster M 3”. Bulletin of the Astronomical Institutes of the Netherlands. 5: 67. Bibcode:1929BAN.....5...67W.
  2. ↑ Morgan, William Wilson; Keenan, Philip Childs; Kellman, Edith (1943). “An atlas of stellar spectra, with an outline of spectral classification”. Chicago. Bibcode:1943assw.book.....M.
  3. ↑ De Jager, Cornelis (1980). “The Main Observational Characteristics of the Most Luminous Stars”. The Brightest Stars. tr. 18. doi:10.1007/978-94-009-9030-2_2. ISBN 978-90-277-1110-6.
  4. ↑ Llorente De Andres, F.; Lamers, H. J. G. L. M.; Muller, E. A. (1979). “Line Blocking in the Near Ultraviolet Spectrum of Early-Type Stars - Part Two - the Dependence on Spectral Type and Luminosity for Normal Stars”. Astronomy and Astrophysics Supplement. 38: 367. Bibcode:1979A&AS...38..367L.
  5. 1 2 Zsoldos, E.; Percy, J. R. (1991). “Photometry of yellow semiregular variables - Rho Cassiopeiae”. Astronomy and Astrophysics. 246: 441. Bibcode:1991A&A...246..441Z. ISSN 0004-6361.
  6. ↑ De Jager, Cornelis; Nieuwenhuijzen, Hans (1992). “Yellow hypergiant interferometry: A clue to understanding evolutionary instability”. In ESA. 344: 109. Bibcode:1992ESASP.344..109D.
  7. ↑ Achmad, L.; Lamers, H. J. G. L. M.; Nieuwenhuijzen, H.; Van Genderen, A. M. (1992). “A photometric study of the G0-4 Ia(+) hypergiant HD 96918 (V382 Carinae)”. Astronomy and Astrophysics. 259: 600. Bibcode:1992A&A...259..600A. ISSN 0004-6361.
  8. ↑ Napiwotzki, R.; Schoenberner, D.; Wenske, V. (1993). “On the determination of effective temperature and surface gravity of B, A, and F stars using Stromgren UVBY beta photometry”. Astronomy and Astrophysics. 268: 653. Bibcode:1993A&A...268..653N. ISSN 0004-6361.
  9. ↑ Arellano Ferro, A.; Giridhar, S.; Rojo Arellano, E. (2003). “A Revised Calibration of the MV-W(O I 7774) Relationship using Hipparcos Data: Its Application to Cepheids and Evolved Stars”. Revista Mexicana de Astronomía y Astrofísica. 39: 3. arXiv:astro-ph/0210695. Bibcode:2003RMxAA..39....3A.
  10. 1 2 3 4 5 De Jager, C. (1998). “The yellow hypergiants”. Astronomy and Astrophysics Review. 8 (3): 145–180. Bibcode:1998A&ARv...8..145D. doi:10.1007/s001590050009.
  11. ↑ Lobel, A.; De Jager, K.; Nieuwenhuijzen, H. (2013). “Long-term Spectroscopic Monitoring of Cool Hypergiants HR 8752, IRC+10420, and 6 Cas near the Yellow Evolutionary Void”. 370 Years of Astronomy in Utrecht. Proceedings of a conference held 2–5 April. 470: 167. Bibcode:2013ASPC..470..167L.
  12. ↑ Humphreys, Roberta M.; Davidson, Kris; Grammer, Skyler; Kneeland, Nathan; Martin, John C.; Weis, Kerstin; Burggraf, Birgitta (2013). “Luminous and Variable Stars in M31 and M33. I. The Warm Hypergiants and Post-Red Supergiant Evolution”. The Astrophysical Journal. 773: 46. arXiv:1305.6051. Bibcode:2013ApJ...773...46H. doi:10.1088/0004-637X/773/1/46.
  13. ↑ Shenoy, Dinesh; Humphreys, Roberta M.; Jones, Terry J.; Marengo, Massimo; Gehrz, Robert D.; Helton, L. Andrew; Hoffmann, William F.; Skemer, Andrew J.; Hinz, Philip M. (2016). “Searching for Cool Dust in the Mid-to-far Infrared: The Mass-loss Histories of the Hypergiants μ Cep, VY CMa, IRC+10420, and ρ Cas”. The Astronomical Journal. 151 (3): 51. arXiv:1512.01529. Bibcode:2016AJ....151...51S. doi:10.3847/0004-6256/151/3/51.
  14. 1 2 3 Stothers, R. B.; Chin, C. W. (2001). “Yellow Hypergiants as Dynamically Unstable Post–Red Supergiant Stars”. The Astrophysical Journal. 560 (2): 934. Bibcode:2001ApJ...560..934S. doi:10.1086/322438.
  15. 1 2 3 Nieuwenhuijzen, H; de Jager, C (2000). “Checking the yellow evolutionary void. Three evolutionary critical Hypergiants: HD 33579, HR 8752 & IRC +10420”. Astronomy and Astrophysics. 353: 163–176. Bibcode:2000A&A...353..163N.Nieuwenhuijzen, H.; De Jager, C. (2000). “Checking the yellow evolutionary void. Three evolutionary critical Hypergiants: HD 33579, HR 8752 & IRC +10420”. Astronomy and Astrophysics. 353: 163. Bibcode:2000A&A...353..163N.
  16. ↑ Lobel, A.; Israelian, G.; de Jager, C.; Musaev, F.; Parker, J. W.; Mavrogiorgou, A. (1998). “The spectral variability of the cool hypergiant rho Cassiopeiae”. Astronomy and Astrophysics. 330: 659–675. Bibcode:1998A&A...330..659L.
  17. ↑ Lobel; Stefanik; Torres; Davis; Ilyin; Rosenbush (2003). “Spectroscopy of the Millennium Outburst and Recent Variability of the Yellow Hypergiant Rho Cassiopeiae”. Stars as suns: activity. 219: 903. arXiv:astro-ph/0312074. Bibcode:2004IAUS..219..903L.
  18. ↑ Groh, Jose H.; Meynet, Georges; Georgy, Cyril; Ekström, Sylvia (2013). “Fundamental properties of core-collapse supernova and GRB progenitors: Predicting the look of massive stars before death”. Astronomy & Astrophysics. 558: A131. arXiv:1308.4681. Bibcode:2013A&A...558A.131G. doi:10.1051/0004-6361/201321906.
  19. ↑ Gesicki, K. (1992). “A Modelling of Circumstellar BAII Lines for the Hypergiant Rho-Cassiopeiae”. Astronomy and Astrophysics. 254: 280. Bibcode:1992A&A...254..280G.
  20. ↑ Langer, N.; Norman, C. A.; De Koter, A.; Vink, J. S.; Cantiello, M.; Yoon, S. -C. (2007). “Pair creation supernovae at low and high redshift”. Astronomy and Astrophysics. 475 (2): L19. arXiv:0708.1970. Bibcode:2007A&A...475L..19L. doi:10.1051/0004-6361:20078482.
  21. ↑ Georgy, C. (2012). “Yellow supergiants as supernova progenitors: An indication of strong mass loss for red supergiants?”. Astronomy & Astrophysics. 538: L8–L2. arXiv:1111.7003. Bibcode:2012A&A...538L...8G. doi:10.1051/0004-6361/201118372.
  22. ↑ Maund, J. R.; Fraser, M.; Ergon, M.; Pastorello, A.; Smartt, S. J.; Sollerman, J.; Benetti, S.; Botticella, M. -T.; Bufano, F. (2011). “The Yellow Supergiant Progenitor of the Type II Supernova 2011dh in M51”. The Astrophysical Journal. 739 (2): L37. arXiv:1106.2565. Bibcode:2011ApJ...739L..37M. doi:10.1088/2041-8205/739/2/L37.
  23. ↑ Groh, Jose H. (2014). “Early-time spectra of supernovae and their precursor winds”. Astronomy & Astrophysics. 572: L11. arXiv:1408.5397. Bibcode:2014A&A...572L..11G. doi:10.1051/0004-6361/201424852.
  24. ↑ Smith, N.; Vink, J. S.; De Koter, A. (2004). “The Missing Luminous Blue Variables and the Bistability Jump”. The Astrophysical Journal. 615: 475. arXiv:astro-ph/0407202. Bibcode:2004ApJ...615..475S. doi:10.1086/424030.
  25. ↑ Chieffi, Alessandro; Limongi, Marco (2013). “Pre-Supernova Evolution of Rotating Solar Metallicity Stars in the Mass Range 13-120M☉And Their Explosive Yields”. The Astrophysical Journal. 764: 21. Bibcode:2013ApJ...764...21C. doi:10.1088/0004-637X/764/1/21.
  26. ↑ Fadeyev, Y. A. (2011). “Pulsational instability of yellow hypergiants”. Astronomy Letters. 37 (6): 403–413. arXiv:1102.3810. Bibcode:2011AstL...37..403F. doi:10.1134/S1063773711060016.
  27. ↑ Langer, Norbert; Heger, Alexander; García-Segura, Guillermo (1998). “Massive Stars: The Pre-Supernova Evolution of Internal and Circumstellar Structure”. Reviews in Modern Astronomy 11: Stars and Galaxies. Hamburg. 11: 57. Bibcode:1998RvMA...11...57L.
  28. ↑ Dinh-v-Trung; Muller, S. B.; Lim, J.; Kwok, S.; Muthu, C. (2009). “Probing the Mass-Loss History of the Yellow Hypergiant IRC+10420”. The Astrophysical Journal. 697: 409. arXiv:0903.3714. Bibcode:2009ApJ...697..409D. doi:10.1088/0004-637X/697/1/409.
  29. ↑ Lagadec, E.; Zijlstra, A. A.; Oudmaijer, R. D.; Verhoelst, T.; Cox, N. L. J.; Szczerba, R.; Mékarnia, D.; Van Winckel, H. (2011). “A double detached shell around a post-red supergiant: IRAS 17163-3907, the Fried Egg nebula”. Astronomy & Astrophysics. 534: L10. arXiv:1109.5947. Bibcode:2011A&A...534L..10L. doi:10.1051/0004-6361/201117521.
  30. ↑ Benaglia, P.; Vink, J. S.; Martí, J.; Maíz Apellániz, J.; Koribalski, B.; Crowther, P. A. (2007). “Testing the predicted mass-loss bi-stability jump at radio wavelengths”. Astronomy and Astrophysics. 467 (3): 1265. arXiv:astro-ph/0703577. Bibcode:2007A&A...467.1265B. doi:10.1051/0004-6361:20077139.
  31. ↑ Clark, J. S.; Negueruela, I.; González-Fernández, C. (2013). “IRAS 18357-0604 – an analogue of the galactic yellow hypergiant IRC +10420?”. Astronomy & Astrophysics. 561: A15. arXiv:1311.3956. Bibcode:2014A&A...561A..15C. doi:10.1051/0004-6361/201322772.
  32. ↑ Wittkowski, M.; Arroyo-Torres, B.; Marcaide, J. M.; Abellan, F. J.; Chiavassa, A.; Guirado, J. C. (2017). “VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), σ Oph, BM Sco, and HD 206859”. Astronomy & Astrophysics. 597: A9. arXiv:1610.01927. Bibcode:2017A&A...597A...9W. doi:10.1051/0004-6361/201629349.
  33. ↑ Davies, Ben; Figer, Don F.; Law, Casey J.; Kudritzki, Rolf‐Peter; Najarro, Francisco; Herrero, Artemio; MacKenty, John W. (2008). “The Cool Supergiant Population of the Massive Young Star Cluster RSGC1”. The Astrophysical Journal. 676 (2): 1016–1028. arXiv:0711.4757. Bibcode:2008ApJ...676.1016D. doi:10.1086/527350.
  34. ↑ Clark, J. S.; Negueruela, I.; Crowther, P. A.; Goodwin, S. P. (2005). “On the massive stellar population of the super star cluster Westerlund 1”. Astronomy and Astrophysics. 434 (3): 949. arXiv:astro-ph/0504342. Bibcode:2005A&A...434..949C. doi:10.1051/0004-6361:20042413.
  35. 1 2 Humphreys, R. M.; Weis, K.; Davidson, K.; Bomans, D. J.; Burggraf, B. (2014). “LUMINOUS AND VARIABLE STARS IN M31 AND M33. II. LUMINOUS BLUE VARIABLES, CANDIDATE LBVs, Fe II EMISSION LINE STARS, AND OTHER SUPERGIANTS”. The Astrophysical Journal. 790: 48. arXiv:1407.2259. Bibcode:2014ApJ...790...48H. doi:10.1088/0004-637X/790/1/48.
Pulsating
Biến quang Cepheid and
cepheid-like
Blue-white with
early spectra
Long-period
Other


Eruptive
Tiền sao Tiền dãy chính
Giants and
supergiants
Eruptive binary
Other
Cataclysmic
Rotating
Non-spherical
Stellar spots
Magnetic fields
Eclipsing