Non-Radial Oscillations in CV Primaries

Details Non-Radial Oscillations in CV Primaries Non-Radial Oscillations in CV Primaries

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..334..453w&link_type=abstract

14th European Workshop on White Dwarfs, ASP Conference Series, Vol. 334 Proceedings of a meeting held at Kiel, July 19-23, 2004

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We review current knowledge of ZZ Cet-type non-radial oscillations in
the white dwarf primaries of cataclysmic variable stars. There are five
definite and two possible systems known so far, the majority have been
found from the Sloan Digital Sky Survey.

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