XMM-Newton Proposal 03059807

Details XMM-Newton Proposal 03059807 XMM-Newton Proposal 03059807

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..196n&link_type=abstract

XMM-Newton Proposal ID #03059807

Other

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Wd 0232+035, Bpm 71214, Rr Cae, Uz Sex, Eg Uma, Wd 1541-381, Xmm-Newton Proposal 03059807

Scientific paper

We propose a systematic investigation of the stellar activity of M dwarfs in a sample of close binary systems with a white dwarf companion. We will use the X-ray flux as tracer of stellar activity and measure its dependence on the rotational periods. A comparison with results for single stars from the literature will assess whether both classes of M dwarfs follow the same relation. This will test whether the current concept of magnetic braking in close binaries is valid. Our results will have implications for many other types of close binary systems

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