Varieties of WN star X-ray Emission Mechanisms

Details Varieties of WN star X-ray Emission Mechanisms Varieties of WN star X-ray Emission Mechanisms

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..192p&link_type=abstract

XMM-Newton Proposal ID #05562603

Physics

Stars, White Dwarfs, Solar System, Wr 133, Xmm-Newton Proposal Id #05562603

Scientific paper

The extreme range of physical conditions in the winds of Wolf-Rayet stars of the nitrogen sequence in terms of density, velocity and chemical composition gives more leverage to attack the unsolved origin of X-rays from hot stars than available through the more homogenous O stars. We propose to obtain EPIC spectra of 4 prominent WN stars, including two single stars and two binaries, in order to explore both ends of the luminosity distribution.

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