X-ray Eclipses in the 2010 January Outburst of the Recurrent Nova U Sco?

Details X-ray Eclipses in the 2010 January Outburst of the Recurrent Nova U Sco? X-ray Eclipses in the 2010 January Outburst of the Recurrent Nova U Sco?

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21733813m&link_type=abstract

American Astronomical Society, AAS Meeting #217, #338.13; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

The recurrent nova 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.

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