@article {22759,
	title = {On the Role of Radioactive Decays in Powering Gamma Rays and X-Rays from Novae},
	volume = {394},
	year = {1992},
	month = {1992/07/1},
	pages = {217},
	abstract = {Existing models for X-ray emission from novae in outburst encounter several difficulties. The X-ray flux that may be expected to result from Compton degradation of gamma rays produced by radioactive decays is calculated. It is demonstrated that radioactive decays of Na-22 may play an interesting role in the production of hard X-rays, particularly in novae enriched in oxygen, neon, and magnesium.},
	keywords = {Abundances, Astrophysics, CATACLYSMIC VARIABLES, Gamma Ray Astronomy, Light Curve, Novae, Nuclear Astrophysics, Nuclear Fusion, Nuclear Reactions, Nucleosynthesis, Radioactive Decay, Sodium 22, STARS: NOVAE, stellar evolution, Stellar Models, X Ray Stars, X-Rays: Stars},
	isbn = {0004-637X},
	url = {https://ui.adsabs.harvard.edu/abs/1992ApJ...394..217L},
	author = {Livio, Mario and Mastichiadis, Apostolos and Oegelman, Hakki and Truran, James W.}
}
