HYDROGEN-POOR CIRCUMSTELLAR SHELLS FROM PULSATIONAL PAIR-INSTABILITY SUPERNOVAE WITH RAPIDLY ROTATING PROGENITORS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/760/i=2/a=154/pdf
Reference41 articles.
1. Dynamics of Supernova Explosion Resulting from Pair Formation
2. EFFECTS OF ROTATION ON THE MINIMUM MASS OF PRIMORDIAL PROGENITORS OF PAIR-INSTABILITY SUPERNOVAE
3. GENERALIZED SEMI-ANALYTICAL MODELS OF SUPERNOVA LIGHT CURVES
4. Self-similar solutions for the interaction of stellar ejecta with an external medium
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