Binary White Dwarfs is a stellar system consisting of two white dwarf stars gravitationally bound in a close orbit, distinguished from single white dwarfs and other binary systems by the degenerate nature and evolutionary endpoint status of both components.
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NORMAL TYPE Ia SUPERNOVAE FROM VIOLENT MERGERS OF WHITE DWARF BINARIES
Rüdiger Pakmor, M. Kromer, S. Taubenberger et al. · The Astrophysical Journal Letters · 2012 · 463 citations · Full text
Natural Sciences, Astronomy, Physics +15
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