Department
of Astronomy, University of Washington, Seattle, WA 98195
Arne Henden
U.S.
Naval Observatory, Flagstaff Station, P.O. Box 1149, Flagstaff, AZ 86002
and
Universities
Space Research Association (currently at AAVSO, 25 Birch Street, Cambridge, MA
02138)
Presented
at the 94th Spring Meeting of the AAVSO, March 25, 2005; received May 19, 2005;
revised June 13, 2005; accepted June 14, 2005
AbstractIn
the four years since the Sloan Digital Sky Survey (SDSS) began operation, over
100 new cataclysmic variables (CV) have been found. Among these are many
interesting systems, including eclipsing, pulsating, and magnetic CVs. A
comparison of the statistics emerging from the observed period distribution of
the SDSS compared to past surveys shows many more short period systems,
consistent with less selection bias based on brightness. Opportunities for
observations with ongoing XMM and HST projects are presented.