Magnetic Accreting White Dwarfs in the XMM-Newton Era

Details Magnetic Accreting White Dwarfs in the XMM-Newton Era Magnetic Accreting White Dwarfs in the XMM-Newton Era

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..151d&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Other

Accretion Disks, X-Ray Sources (Astronomical), Magnetic Fields, White Dwarfs, Infall, Accretion, And Accretion Disks, X-Ray Sources, X-Ray Bursts, Gravitational Radiation, Magnetic Fields, And Other Observations, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

Magnetic Cataclysmic Variables (MCVs) are the brightest X-ray sources among accreting white dwarf binaries. They were recently found to constitute a non-negligible fraction of galactic hard (>20 keV) X-ray sources suggesting a still hidden but potentially important population. XMM-Newton allowed to identify the true nature of many new CV candidates, to infer unexpected X-ray properties and their link with fundamental parameters of the accreting primaries.

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