Gamma-ray emission of classical novae and its detectability by INTEGRAL

Details Gamma-ray emission of classical novae and its detectability by INTEGRAL Gamma-ray emission of classical novae and its detectability by INTEGRAL

1998-12-04

arxiv.org/abs/astro-ph/9812100v1

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, to appear in "3rd INTEGRAL Workshop: The Extreme Universe", Taormina (Italy)

Scientific paper

A lot of information concerning the mechanism of nova explosions will be extracted from the possible future observations with INTEGRAL. In order to be prepared for this task, we are performing detailed models of the gamma-ray emission of classical novae, for a wide range of possible initial conditions. Spectra at different epochs after the explosion and light curves for the different lines (511, 478 and 1275 keV) and the continuum are presented, as well as the detectability distances with INTEGRAL spectrometer SPI. New results related to 18F synthesis related to very recent data of nuclear physics are advanced as preliminary.

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