Physics
Scientific paper
Mar 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...57s&link_type=abstract
XMM-Newton Proposal ID #02010601
Physics
1643+3402, Xmm-Newton Proposal 02010601
Scientific paper
The SW Sex stars are a sub-type of cataclysmic variable (CV) that show optical absorption at phase 0.5, single-peaked emission lines even at high inclination, and orbital periods of 3-5 hours. Several researchers have speculated that SW Sex stars are magnetic CVs, specifically, intermediate polars. The proposed observations will test that speculation by searches for X-ray periods and hard X-ray spectra, two signatures that define the subclass of intermediate polar.
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