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Pulsational pair instability as an explanation for the most luminous supernovae

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Blinnikov,  S.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Woosley, S. E., Blinnikov, S., & Heger, A. (2007). Pulsational pair instability as an explanation for the most luminous supernovae. Nature, 450(7168), 390-392. doi:10.1038/nature06333.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-A8F1-D
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