White dwarf models for type 1 supernovae and quiet supernovae, and presupernova evolution

Details White dwarf models for type 1 supernovae and quiet supernovae, and presupernova evolution White dwarf models for type 1 supernovae and quiet supernovae, and presupernova evolution

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..563n&link_type=abstract

Space Science Reviews, Volume 27, Issue 3-4, pp. 563-570

Computer Science

18

Neutron Stars, Stellar Mass Accretion, Supernovae, White Dwarf Stars, Deflagration, Electron Capture, Helium, High Temperature Gases, Hydrogen, Stellar Models

Scientific paper

Supernova mechanisms in accreting white dwarfs are considered with emphasis on deflagration as a plausible mechanism for producing Type I supernovae and electron captures to form quiet supernovae leaving neutron stars. These outcomes depend on accretion rate of helium, initial mass and composition of the white dwarf. The various types of hydrogen shell burning in the presupernova stage are also discussed.

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