Pulsational pair instability as an explanation for the most luminous supernovae
S. E. WoosleyDepartment of Astronomy and Astrophysics, UCSC, Santa Cruz, California 95064, USA. [email protected]С. И. БлинниковDepartment of Astronomy and Astrophysics, UCSC, Santa Cruz, California 95064, USA,Alexander HegerTheoretical Astrophysics Group, T-6, MS B227, Los Alamos National Laboratory, Los Alamos, New Mexico 87544, USA ,
2007en
ABI
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