Pulsational pair instability as an explanation for the most luminous supernovae. (Q46331700)
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scientific article published in November 2007
Language | Label | Description | Also known as |
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English | Pulsational pair instability as an explanation for the most luminous supernovae. |
scientific article published in November 2007 |
Statements
Pulsational pair instability as an explanation for the most luminous supernovae (English)
S E Woosley
1 November 2007