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Supernova models [electronic resource].

Published:
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy, 1980.
Physical Description:
Pages: 52 : digital, PDF file
Additional Creators:
Lawrence Livermore National Laboratory and United States. Department of Energy. Office of Scientific and Technical Information
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Summary:
Recent progress in understanding the observed properties of Type I supernovae as a consequence of the thermonuclear detonation of white dwarf stars and the ensuing decay of the /sup 56/Ni produced therein is reviewed. Within the context of this model for Type I explosions and the 1978 model for Type II explosions, the expected nucleosynthesis and gamma-line spectra from both kinds of supernovae are presented. Finally, a qualitatively new approach to the problem of massive star death and Type II supernovae based upon a combination of rotation and thermonuclear burning is discussed.
Report Numbers:
E 1.99:ucrl-85575
E 1.99: conf-801250-1
conf-801250-1
ucrl-85575
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Note:
Published through SciTech Connect.
01/01/1980.
"ucrl-85575"
" conf-801250-1"
10. Texas symposium on relativistic astrophysics, Baltimore, MD, USA, 15 Dec 1980.
Weaver, T.A.; Woosley, S.E.
California Univ., Santa Cruz (USA)
Funding Information:
W-7405-ENG-48
View MARC record | catkey: 13827882