X-ray properties of newly identified magnetic Cataclysmic Variables

Details X-ray properties of newly identified magnetic Cataclysmic Variables X-ray properties of newly identified magnetic Cataclysmic Variables

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop...63d&link_type=abstract

XMM-Newton Proposal ID #04016502

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Rxj0704+2625, Rxj1803+4012, Xmm-Newton Proposal 04016502

Scientific paper

New optically identified Cataclysmic Variables (CVs) have recently increased as candidates the number of Intermediate Polar systems making them nowdays a conspicuous and important class for the study of the evolution of magnetic CVs. Among 15 candidates representing about 50% of the class, we propose to observe five new systems recently found to be strong optical pulsators. The detection of X-ray pulses at the white dwarf spin period and their spectral properties will provide firm constraints on their true magnetic nature thus helping in reconciling the still fragmentary picture of accretion and evolution of magnetic CVs.

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