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- W1618846551 abstract "The recent satellite observations of the 1.8 MeV line from the decay of Al-26 has given a new impetus to the study of the nucleosynthesis of Al-26. The production and ejection of Al-26 by massive mass-losing stars (Of and WR stars) is discussed in the light of recent stellar models. The longitude distribution of the Al-26 gamma ray line emission produced by the galactic collection of WR stars is derived based on various estimates of their radial distribution. This longitude profile provides: (1) a specific signature of massive stars on the background of other potential Al-26 sources, as novae, supernovae, certain red giants and possibly AGB stars; and (2) a possible tool to improve the data analysis of the HEAO 3 and SMM experiments." @default.
- W1618846551 created "2016-06-24" @default.
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- W1618846551 date "1985-08-01" @default.
- W1618846551 modified "2023-09-23" @default.
- W1618846551 title "Gamma-ray line emission from Al-26 produced by Wolf-Rayet stars" @default.
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