Hard emission from classical novae

Details Hard emission from classical novae Hard emission from classical novae

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..299l&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 299-301.

Astronomy and Astrophysics

Astrophysics

9

Emission Spectra, Novae, Nuclear Astrophysics, White Dwarf Stars, X Ray Stars, Gamma Ray Spectra, Star Distribution, Stellar Models, Stellar Spectra, X Ray Spectra

Scientific paper

The thermonuclear model of classical novae has been very successful in explaining many observed features of novae. It also predicts unique gamma-ray and X-ray signatures, a few of which possibly have already been observed. We describe recent developments in the expectations of these signatures and we discuss prospects for additional observations with current observatories.

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