γ-rays from classical novae: expectations from present and future missions

Details γ-rays from classical novae: expectations from present and future missions γ-rays from classical novae: expectations from present and future missions

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newar..48...35h&link_type=abstract

New Astronomy Reviews, Volume 48, Issue 1-4, p. 35-39.

Astronomy and Astrophysics

Astronomy

13

Γ-Ray Astronomy, Γ-Ray Lines, Nucleosynthesis, Novae, Cataclysmic Variables

Scientific paper

A review of the main features of the γ-ray emission of individual classical novae is presented. We concentrate on the theoretical predictions of both the long lasting emission, produced by electron captures on 7Be and β+-decay of 22Na, and the prompt emission, produced by electron-positron annihilation (with positrons coming from 13N and 18F β+-decays). Special attention is paid to the observability of novae with the current INTEGRAL observatory and with future missions, like EXIST.

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