Supernovae pp 595-598 | Cite as
Collapse or Explosion of C+O White Dwarfs
Conference paper
Abstract
The existence and the orbital parameters of low-mass binary x-ray sources suggest that a fraction at least of neutron stars have been produced by the accretion induced collapse (AIC) of a white dwarf (TAAM and VAN DEN HEUVEL [1]). Two types of candidates have been proposed thus far: carbon-oxygen white dwarfs (CANAL and SCHATZMANN [2]; CANAL and ISERN [3]; CANAL, ISERN and LABAY [4]), and oxygen-neon-magnesium white dwarfs (MIYAJI et al [5]; MIYAJI and NOMOTO [6]).
Keywords
Neutron Star Conductive Velocity White Dwarf Fluid Layer Front Velocity
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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© Springer-Verlag New York, Inc. 1991