Using XMM-Newton and Optical Photometry to Figure Out CVs

Details Using XMM-Newton and Optical Photometry to Figure Out CVs Using XMM-Newton and Optical Photometry to Figure Out CVs

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006javso..35..306s&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 35, no. 1, p. 306-310

Physics

Xmm-Newton, Photometry, Cataclysmic Variables

Scientific paper

X-ray light curves from XMM-Newton combined with optical data from the satellite and ground-based observers provide distinctive shapes and periodicities that give information on the correct classification of cataclysmic variables. Our recent data on three SDSS sources with strong helium emission are used to identify a highly magnetic system (a polar), the spin of the white dwarf in an intermediate polar, and a typical disk accreting system.

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