XMM-Newton Proposal 03055701

Details XMM-Newton Proposal 03055701 XMM-Newton Proposal 03055701

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..178g&link_type=abstract

XMM-Newton Proposal ID #03055701

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Hs2331+3905, Xmm-Newton Proposal 03055701

Scientific paper

We have recently identified the cataclysmic variable (CV) HS2331+3905, which displays a fascinating combination of properties: it is probably one of the oldest known CVs with a brown dwarf donor, it is brightest CV containing a pulsating white dwarf which is probably rotating with a very short spin period of 67s, and it may harbour a precessing warped accretion disc. We have already explored this system from the ultraviolet into the infrared, and request here XMM-Newton time to unambiguously determine whether the white dwarf in HS2331+3905 is a magnetic rapid rotator.

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