Searching for double degenerates.

Details Searching for double degenerates. Searching for double degenerates.

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988msngr..52...35b&link_type=abstract

The Messenger, vol. 52, p. 35-39

Physics

10

Degenerate Stars:Detection, Spectra:White Dwarfs, White Dwarfs:Spectra

Scientific paper

The majority of stars are members of binary systems; this is a frequently referred aphorism. The majority of stars also terminate their evolution as white dwarfs (WDs), as only few stars are born massive enough to experience a supernova explosion. We can easily conclude that the majority of binary systems must at some stage become a double WD binary, and that a good fraction of the stars listed in our catalogues as WDs may indeed be double.

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