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2008ApJ...685.1103W - Astrophys. J., 685, 1103-1108 (2008/October-1)
The most massive core-collapse supernova progenitors.
WALDMAN R.
Abstract (from CDS):
The discovery of the extremely luminous supernova SN 2006gy, possibly interpreted as a pair instability supernova, renewed the interest in very massive stars. We explore the evolution of these objects, which end their life as pair instability supernovae or as core-collapse supernovae with relatively massive iron cores, up to about 3 M☉.
Abstract Copyright: ∼
Journal keyword(s): Stars: Evolution - Stars: Supernovae: General
Simbad objects: 1
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