Li-7 gamma-ray lines from novae

Details Li-7 gamma-ray lines from novae Li-7 gamma-ray lines from novae

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...244l..97c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 244, Mar. 1, 1981, p. L97, L98.

Astronomy and Astrophysics

Astronomy

24

Gamma Ray Astronomy, Lithium Isotopes, Novae, Nuclear Fusion, Stellar Radiation, Gamma Ray Observatory, Gamma Ray Spectra

Scientific paper

The possible nucleosynthetic origins of the Li-7 abundance in nova explosions is discussed. The observation of the 478 keV gamma-ray line emitted as Be-7 decays to Li-7 in the expanding ejecta is shown to provide an opportunity to test this hypothesis as well as nova theory. It is noted that the anticipated flux, 10,000 sq cm/sec at 1 kpc, is within range of the Gamma-Ray Observatory.

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