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.

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