Variable strong X-ray emission lines in U Sco

Details Variable strong X-ray emission lines in U Sco Variable strong X-ray emission lines in U Sco

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2469....1n&link_type=abstract

The Astronomer's Telegram, #2469

Astronomy and Astrophysics

Astronomy

2

X-Ray, Cataclysmic Variables, Novae

Scientific paper

An XMM-Newton observation of the eclipsing, recurrent nova U Sco was carried out, yielding a high-resolution X-ray spectrum. The observation with the Reflection Grating Spectrometer (RGS) started 2010-02-19T15:41:09 (=22.23 days after discovery) and ended 2010-02-20T09:24:41. During the exposure time of 63360s, an average count rate of 1 count per second (cps) was observed with variations between 0.5 and 1.5 cps.

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