XMM-Newton Proposal 03021002

Details XMM-Newton Proposal 03021002 XMM-Newton Proposal 03021002

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...71d&link_type=abstract

XMM-Newton Proposal ID #03021002

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Rxj2133.7+5107, Rxj1730.7-0559, Xmm-Newton Proposal 03021002

Scientific paper

We propose five X-ray selected Cataclysmic Variables which, for their large optical pulsations, are strong candidates of being members of the magnetic Intermediate Polar class. We aim to confirm their true nature by detecting X-ray pulses at the white dwarf spin period and determining their spectral properties. These systems cover a wide range of asynchronism and soft-to-hard X-ray ratios and represent 20% of the entire class, thus a potential for our understanding of accretion and evolution of magnetic Cataclysmic Variables.

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