paper

Type Ia Supernovae and Remnant Neutron Stars

arXiv:astro-ph/0011150 · doi:10.1046/j.1365-8711.2001.04184.x

Abstract

On the basis of the current observational evidence, we put forward the case that the merger of two CO white dwarfs produces both a Type Ia supernova explosion and a stellar remnant, the latter in the form of a magnetar. The estimated occurrence rates raise the possibility that many, if not most, SNe Ia might result from white dwarf mergers.

4 pages, no figures; accepted for MNRAS; typo corrected

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