RS Ophiuchi in outburst, seen with XMM-Newton and Chandra

Details RS Ophiuchi in outburst, seen with XMM-Newton and Chandra RS Ophiuchi in outburst, seen with XMM-Newton and Chandra

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...4e..17o&link_type=abstract

The Ultraviolet Universe: Stars from Birth to Death, 26th meeting of the IAU, Joint Discussion 4, 16-17 August 2006, Prague, Cze

Physics

Scientific paper

RS Ophiuchi, a peculiar recurrent nova that is thought to be a possible type Ia N candidate, had its sixth recorded outburst since 1898 this year. It wa simemdiately monitored with many different instuments including All available X-ray telescopes. We present the behaviour of X-ray Ophiuchi at the softest X-ray energies, close to EUV, at the time at which the envelope becomes transparent to the central object, including grating spectra and the light curve in which a puzzling and interesting 35 seconds pulsation can be detected.

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