A XMM-Newton Observation of Nova LMC 1995

Details A XMM-Newton Observation of Nova LMC 1995 A XMM-Newton Observation of Nova LMC 1995

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..355o&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 3

Other

Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, X-Ray Sources, X-Ray Bursts, Magellanic Clouds And Other Irregular Galaxies, Faint Blue Stars, White Dwarfs, Degenerate Stars, Nuclei Of Planetary Nebulae

Scientific paper

Nova LMC 1995, detected as a luminous supersoft X-ray source in 1995-1998 with ROSAT, was observed again in December of 2000 with XMM-Newton. It was still a supersoft X-ray source at almost-Eddington luminosity, and the effective temperature had increased to about 450,000 K. We discuss atmospheric models studied for the hot hydrogen burning white dwarf, and whether this nova may be a type Ia supernova progenitor.

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