Other
Scientific paper
Mar 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005soust..44a..24w&link_type=abstract
Southern Stars. The Journal of the Royal Astronomical Society of New Zealand (ISSN 0049-1640), Vol. 44, No. 1, p. 24 - 27 (2005)
Other
Scientific paper
To start, let me remind you that cataclysmic variables form one of the types of interacting binary star (or close binary) wherein mass is transferred from one star to another. If the accreting component is a degenerate star then the term compact binary is usually used - the accretor may be a white dwarf, a neutron star or a black hole. The donor can also be almost any sort of star - main sequence, giant, supergiant or even another white dwarf.
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