"Gamma-Ray Lines: A 22Na Radioactive Diagnostic of Young Supernovae" by Donald D. Clayton
 

Document Type

Article

Publication Date

5-15-1975

Publication Title

The Astrophysical Journal

Publisher

The American Astronomical Society

Abstract

The nuclear y-ray lines emitted following the decay of 22Na should be detectable for roughly a decade following Galactic explosions of massive stars in which the helium shell is heated sufficiently to synthesize 19F and 21Ne from seed 14N.

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