Document Type
Article
Publication Date
6-9-1992
Publication Title
Astronomy & Astrophysics
Publisher
EDP Sciences
Abstract
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.
Recommended Citation
Please use publisher's recommended citation.
COinS