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White Dwarf Models for Type I Supernovae and Quiet Supernovae, and Presupernova Evolution

Published online by Cambridge University Press:  12 April 2016

Ken’ichi Nomoto
Ken’ichi Nomoto*
Affiliation:
Laboratory for Astronomy and Solar Physics NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA

Abstract

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Supernova mechanisms in accreting white dwarfs (WDs) are presented, i.e., the carbon 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 WD. The various types of hydrogen shell-burning in the présupernova stage are also discussed.

Type
IX. Supernovae
Information
International Astronomical Union Colloquium , Volume 58: Stellar Hydrodynamics , August 1980 , pp. 563 - 570
Copyright
Copyright © Reidel 1980

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