Gamma‐ray line diagnostics of Novae
2008
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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