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, Type Ia supernovae might result from white dwarf mergers.
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King, A. R., Pringle, J. E., & Wickramasinghe, D. T. (2001). Type Ia supernovae and remnant neutron s tars. Monthly Notices of the Royal Astronomical Society, 320(3), L45–L48. https://doi.org/10.1046/j.1365-8711.2001.04184.x
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