White dwarf pairing functions

Details White dwarf pairing functions White dwarf pairing functions

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1273..378f&link_type=abstract

17TH EUROPEAN WHITE DWARF WORKSHOP. AIP Conference Proceedings, Volume 1273, pp. 378-383 (2010).

Computer Science

White Dwarfs, Binary Stars, Spectroscopy, Stellar Mass, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae, X-Ray Binaries, Spectroscopy And Spectrophotometry, Masses

Scientific paper

In the local volume limited sample of white dwarfs, some 12% are found paired with M dwarfs. However, there are no known high field magnetic white dwarfs with a detached M dwarf companion. Such pairings also seem to be uncommon in the general class of massive white dwarfs, regardless of whether they are strongly magnetic or not. Taking note of the fact that high field magnetic white dwarfs tend to have high-mass progenitors, we investigate the possibility that the above result may be a direct consequence of the manner in which stars form and pair on the main sequence.

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