Physics
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aps..tsffp1019v&link_type=abstract
American Physical Society, Joint Fall 2010 Meeting of the Texas Sections of the APS, AAPT, Zone 13 of SPS and the National Socie
Physics
Scientific paper
The recurrent nova U Scorpius (U Sco) is an eclipsing system with an orbit inclination of 80-83 degrees and for which the secondary blocks the light from the primary for ˜0.1 of the orbit in the optical. A clean test of the origin of the X-ray flux in the burst is made possible by U Sco: if X-rays arise from the proximity of the white dwarf, then we must detect X-ray eclipses and the exact shape of the eclipse determines the nature of the distribution of emitting matter. We describe the comparison of X-ray spectra obtained in and out of eclipse.
Engelhardt Sabrina
McMaster Laura
Moore Marilyn
Pagnotta Ashley
Schlegel Eric
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