X-ray observations of classical novae during the outburst stage by EXOSAT

Details X-ray observations of classical novae during the outburst stage by EXOSAT X-ray observations of classical novae during the outburst stage by EXOSAT

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..177o&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 177-179 (SEE N86-20287 10-93)

Astronomy and Astrophysics

Astronomy

2

Exosat Satellite, Novae, Stellar Radiation, X Ray Astronomy, Spaceborne Astronomy, Stellar Models, White Dwarf Stars, X Ray Absorption, X Rays

Scientific paper

Soft X-ray observations of Nova Mus 83 and Nova Vul 84(1) by EXOSAT are described. Nova Mus 83 continues to emit X-rays 18 and 23 months after the outburst at the same intensity as the original observation 15 months after outburst. Nova Vul 84(1) was observed at optical maximum and not detected; a second observation three months later yields a 2 sigma signal. The results are discussed in terms of the possible origin of the X-rays. A hot white dwarf model is suggested.

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