Models for Type I supernovae [electronic resource].
- Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy, 1980.
- Physical Description:
- Pages: 19 : digital, PDF file
- Additional Creators:
- United States. Department of Energy. Office of Scientific and Technical Information
- Restrictions on Access:
- Free-to-read Unrestricted online access
- Two rather disjoint scenarios for Type I supernovae are presented. One is based upon mass accretion by a white dwarf in a binary system. The second involves a star having some 8 to 10 times the mass of the sun which may or may not be a solitary star. Despite the apparent dissimilarities in the models it may be that each occurs to some extent in nature for they both share the possibility of producing substantial quantities of /sup 56/Ni and explosions in stars devoid of hydrogen envelopes. These are believed to be two properties that must be shared by any viable Type I model.
- Report Numbers:
- E 1.99:ucrl-84544
E 1.99: conf-800480-3
- Published through SciTech Connect.
ASCOT program planning meeting, Gettysburg, PA, USA, 15 Apr 1980.
Weaver, T.A.; Woosley, S.E.; Taam, R.E.
California Univ., Livermore (USA). Lawrence Livermore Lab.
- Funding Information:
View MARC record | catkey: 13828761