Theoretical models for supernovae

Details Theoretical models for supernovae Theoretical models for supernovae

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8316268w&link_type=abstract

Presented at the NATO/Adv. Study Inst. on Supernovae, Cambridge, United Kingdom, 28 Jun. - 10 Jul. 1981

Astronomy and Astrophysics

Astronomy

Astronomical Models, Mathematical Models, Nuclear Fusion, Supernovae, Black Holes (Astronomy), Carbon, Helium Isotopes, Ignition, Nitrogen Isotopes

Scientific paper

The results of numerical simulations of supernova explosions are presented. Particular emphasis is given to: (1) the nucleosynthesis expected from intermediate mass (10sub solar or = M or = 100 Msub solar) Type II supernovae and detonating white dwarf models for Type I supernovae; (2) a realistic estimate of the gamma-line fluxes expected from this nucleosynthesis; (3) the continued evolution, in one and two dimensions, of intermediate mass stars wherein iron core collapse does not lead to a strong, mass-ejecting shock wave; and (4) the evolution and explosion of vary massive stars (M 100 Msub solar of both Population I and III.

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