Gamma-ray line diagnostics of Novae

Details Gamma-ray line diagnostics of Novae Gamma-ray line diagnostics of Novae

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aipc..170..130l&link_type=abstract

AIP Conference Proceedings, Volume 170, pp. 130-135 (1988).

Physics

3

Supernovae, Elementary Particle Processes, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

The nuclear processing thought to power classical nova outbursts produces substantial quantities of unstable nuclei. These nuclei emit γ-rays and β+'s which might be detectable to present and future γ-ray spectrometers. We discuss the importance of detection of γ-rays for improving our understanding of the nova phenomenon and we review the observations made to date.

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