อ้างอิง ของ มหานวดาราประเภท 1เอ

  1. ↑ Krause, Oliver; Tanaka, Masaomi; Usuda, Tomonori; Hattori, Takashi; Goto, Miwa; Birkmann, Stephan; Nomoto, Ken'ichi (2008-10-28). "Tycho Brahe's 1572 supernova as a standard type Ia explosion revealed from its light echo spectrum". arXiv.org. สืบค้นเมื่อ 2008-12-06.CS1 maint: multiple names: authors list (link)
  2. 1 2 Yoon, S.-C.; Langer, L. (2004). "Presupernova Evolution of Accreting White Dwarfs with Rotation". Astronomy and Astrophysics. 419 (2): 623. doi:10.1051/0004-6361:20035822. สืบค้นเมื่อ 2007-05-30.CS1 maint: multiple names: authors list (link)
  3. 1 2 Mazzali, P. A.; K. Röpke, F. K.; Benetti, S.; Hillebrandt, W. (2007). "A Common Explosion Mechanism for Type Ia Supernovae". Science. 315 (5813): 825–828. doi:10.1126/science.1136259. PMID 17289993. |access-date= requires |url= (help)CS1 maint: multiple names: authors list (link)
  4. 1 2 Khokhlov, A.; Mueller, E.; Hoeflich, P. (1993). "Light curves of Type IA supernova models with different explosion mechanisms". Astronomy and Astrophysics. 270 (1–2): 223–248. สืบค้นเมื่อ 2007-05-22.CS1 maint: multiple names: authors list (link)
  5. ↑ Staff (2006-09-07). "Introduction to Supernova Remnants". NASA Goddard/SAO. สืบค้นเมื่อ 2007-05-01.
  6. ↑ Matheson, Thomas; Kirshner, Robert; Challis, Pete; Jha, Saurabh; และคณะ (2008). "Optical Spectroscopy of Type Ia Supernovae". Astronomical Journal. 135: 1598–1615. doi:10.1088/0004-6256/135/4/1598. สืบค้นเมื่อ 2008-05-19. Explicit use of et al. in: |author= (help)CS1 maint: multiple names: authors list (link)
  7. ↑ da Silva, L. A. L. (1993). "The Classification of Supernovae". Astrophysics and Space Science. 202 (2): 215–236. doi:10.1007/BF00626878. สืบค้นเมื่อ 2008-06-04.
  8. ↑ Lieb, E. H. (1987). "A rigorous examination of the Chandrasekhar theory of stellar collapse". Astrophysical Journal. 323 (1): 140–144. doi:10.1086/165813. สืบค้นเมื่อ 2007-02-01. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  9. ↑ Canal, R. (1997). "The possible white dwarf-neutron star connection". Astrophysics and Space Science Library. 214: 49. สืบค้นเมื่อ 2007-02-01. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  10. ↑ Fryer, C. L.; New, K. C. B. (2006-01-24). "2.1 Collapse scenario". Gravitational Waves from Gravitational Collapse. Max-Planck-Gesellschaft. สืบค้นเมื่อ 2007-06-07.CS1 maint: multiple names: authors list (link)
  11. ↑ Wheeler, J. Craig (2000-01-15). Cosmic Catastrophes: Supernovae, Gamma-Ray Bursts, and Adventures in Hyperspace. Cambridge, UK: สำนักพิมพ์มหาวิทยาลัยเคมบริดจ์. p. 96. ISBN 0521651956.
  12. 1 2 3 4 5 Hillebrandt, W. (2000). "Type IA Supernova Explosion Models". Annual Review of Astronomy and Astrophysics. 38: 191–230. doi:10.1146/annurev.astro.38.1.191. สืบค้นเมื่อ 2007-02-01. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  13. ↑ "Science Summary". ASC / Alliances Center for Astrophysical Thermonuclear Flashes. 2001. สืบค้นเมื่อ 2006-11-27.
  14. 1 2 Röpke, F. K. (2004). "The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in Type Ia supernovae". Astronomy and Astrophysics. 420: L1–L4. doi:10.1051/0004-6361:20040135. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  15. ↑ Gamezo, V. N. (2003-01-03). "Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications". Science. 299 (5603): 77–81. doi:10.1126/science.1078129. PMID 12446871. สืบค้นเมื่อ 2006-11-28. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  16. 1 2 Gilmore, Gerry (2004). "The Short Spectacular Life of a Superstar". Science. 304 (5697): 1915–1916. doi:10.1126/science.1100370. PMID 15218132. สืบค้นเมื่อ 2007-05-01.
  17. ↑ Paczynski, B. (July 28-August 1, 1975). "Common Envelope Binaries". Structure and Evolution of Close Binary Systems. Cambridge, England: Dordrecht, D. Reidel Publishing Co. pp. 75–80. สืบค้นเมื่อ 2007-01-08. Check date values in: |date= (help)
  18. ↑ Postnov, K. A. (2006). "The Evolution of Compact Binary Star Systems". Living Reviews in Relativity. สืบค้นเมื่อ 2007-01-08. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  19. ↑ Staff. "Type Ia Supernova Progenitors". Swinburne University. สืบค้นเมื่อ 2007-05-20.
  20. ↑ "Brightest supernova discovery hints at stellar collision". New Scientist. 2007-01-03. สืบค้นเมื่อ 2007-01-06.
  21. ↑ "The Weirdest Type Ia Supernova Yet". Lawrence Berkeley National Laboratory. 2006-09-20. สืบค้นเมื่อ 2006-11-02.
  22. ↑ "Bizarre Supernova Breaks All The Rules". New Scientist. 2006-09-20. สืบค้นเมื่อ 2007-01-08.
  23. ↑ Whipple, Fred L. (1939). "Supernovae and Stellar Collisions". Proceedings of the National Academy of Sciences of the United States of America. 25 (3): 118–125. doi:10.1073/pnas.25.3.118. สืบค้นเมื่อ 2007-02-01.
  24. ↑ Rubin, V. C. (1999). "A Thousand Blazing Suns: The Inner Life of Globular Clusters". Mercury. 28: 26. สืบค้นเมื่อ 2006-06-02. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  25. ↑ Middleditch, J. (2004). "A White Dwarf Merger Paradigm for Supernovae and Gamma-Ray Bursts". The Astrophysical Journal. 601 (2): L167–L170. doi:10.1086/382074. สืบค้นเมื่อ 2007-02-01.
  26. ↑ Langer, N.; Yoon, S.-C.; Wellstein, S.; Scheithauer, S. (2002). "On the evolution of interacting binaries which contain a white dwarf". ใน Gänsicke, B. T.; Beuermann, K.; Rein, K. (eds.). The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings. San Francisco, California: Astronomical Society of the Pacific. p. 252. สืบค้นเมื่อ 2007-05-25.CS1 maint: multiple names: authors list (link) CS1 maint: uses editors parameter (link)
  27. ↑ van Dyk, Schuyler D. (1992). "Association of supernovae with recent star formation regions in late type galaxies". Astronomical Journal. 103 (6): 1788–1803. doi:10.1086/116195. สืบค้นเมื่อ 2007-02-01.
  28. ↑ Langer, N. (1999). "The evolution of main sequence star + white dwarf binary systems towards Type Ia supernovae". Astronomy and Astrophysics. 362: 1046–1064. สืบค้นเมื่อ 2007-02-01. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  29. ↑ Macri, L. M. (2006). "A New Cepheid Distance to the Maser-Host Galaxy NGC 4258 and Its Implications for the Hubble Constant". Astrophysical Journal. 652 (2): 1133–1149. doi:10.1086/508530. สืบค้นเมื่อ 2007-02-01. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  30. ↑ Colgate, S. A. (1979). "Supernovae as a standard candle for cosmology". Astrophysical Journal. 232 (1): 404–408. doi:10.1086/157300. สืบค้นเมื่อ 2007-02-01.
  31. ↑ Perlmutter, S. (1999). "Measurements of Omega and Lambda from 42 high redshift supernovae" (subscription required). Astrophysical Journal. 517: 565–86. doi:10.1086/307221. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  32. ↑ Riess, Adam G. (1998). "Observational evidence from supernovae for an accelerating Universe and a cosmological constant" (subscription required). Astronomical Journal. 116: 1009–38. doi:10.1086/300499. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  33. ↑ Leibundgut, B. (2001). "A cosmological surprise: the universe accelerates". Europhysics News. 32 (4): 121. doi:10.1051/epn:2001401. สืบค้นเมื่อ 2007-02-01. Unknown parameter |coauthors= ignored (|author= suggested) (help)
  34. ↑ "Confirmation of the accelerated expansion of the Universe". Centre National de la Recherche Scientifique. 2003-09-19. สืบค้นเมื่อ 2006-11-03.
  35. 1 2 3 วิมุติ วสะหลาย. (23 มีนาคม 2553). ซูเปอร์มหานวดารา. สมาคมดาราศาสตร์ไทย. สืบค้น 17-10-2553.
  36. 1 2 Filippenko, A.V. (2004). "Supernovae and Their Massive Star Progenitors". arΧiv:astro-ph/0412029 [astro-ph]. 
  37. ↑ "Type Ib Supernova Spectra". COSMOS - The SAO Encyclopedia of Astronomy. Swinburne University of Technology. สืบค้นเมื่อ 2010-05-05.

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