articleNatureNov 15, 2007GREEN OA

Pulsational pair instability as an explanation for the most luminous supernovae

SES. E. Woosley СИС. И. Блинников AHAlexander Heger

University of California, Santa Cruz · Max Planck Institute for Astrophysics · +1 more institution

Indexed inarxivcrossrefpubmed

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667

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FWCI: 12.80
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References: 39

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Authors

3

SE
S. E. WoosleyCorresponding
University of California, Santa Cruz
СИ
С. И. Блинников
University of California, Santa Cruz, Max Planck Institute for Astrophysics
AH
Alexander Heger
University of California, Santa Cruz, Los Alamos National Laboratory

Topics & keywords

Topics

Keywords

Supernova
Physics
Ejecta
Astrophysics
Astronomy
Stars
Instability
Solar mass

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