Numerical simulations of off-center detonations in helium shells

Details Numerical simulations of off-center detonations in helium shells Numerical simulations of off-center detonations in helium shells

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...370..272l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 370, March 20, 1991, p. 272-281.

Statistics

Computation

52

Computational Astrophysics, Helium, Stellar Envelopes, Supernovae, White Dwarf Stars, Astronomical Models, Stellar Interiors, Temperature Distribution

Scientific paper

The paper presents results of two-dimensional simulations of detonations in helium shells, accreted above various C-O cores. The present calculations confirm results of one-dimensional calculations, showing that a detonation in a heavy helium layer of 0.1-0.3 solar mass, must ignite a detonation in the core, leading to the total disruption of the star (Livne).

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