XMM observations of the supersoft source Nova LMC 1995

Details XMM observations of the supersoft source Nova LMC 1995 XMM observations of the supersoft source Nova LMC 1995

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001tysc.confe.220o&link_type=abstract

Two Years of Science with Chandra, Abstracts from the Symposium held in Washington, DC, 5-7 September, 2001, meeting abstract.

Physics

White Dwarf Binaries And Cataclysmic Variables

Scientific paper

Nova LMC 1995 was the only one among 10 recent LMC novae that appeared as a super-soft X-ray source in the post-outburst years. It was observed with the ROSAT PSPC up to 3 years after the outburst. We show new data, obtained with XMM in December 2000, almost 6 years after the optical eruption. Observations of novae as supersoft X-ray sources have been done only a few times. The new results recently obtained with Chandra and XMM are opening up a new perspective on the characteristics of these sources and their relevance as possible type Ia supernova progenitors.

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