Sub-luminous type Ia supernovae from the mergers of equal-mass white dwarfs with mass ∼0.9M⊙
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Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/nature08642.pdf
Reference29 articles.
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4. Iben, I. & Tutukov, A. V. Supernovae of type I as end products of the evolution of binaries with components of moderate initial mass (M not greater than about 9 solar masses). Astrophys. J. Suppl. Ser. 54, 335–372 (1984)
5. Webbink, R. F. Double white dwarfs as progenitors of R Coronae Borealis stars and type I supernovae. Astrophys. J. 277, 355–360 (1984)
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