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On the source of the Al-26 observed in the interstellar medium
The Astrophysical Journal1985Vol. 288, pp. L21–L21
Citations Over TimeTop 10% of 1985 papers
Abstract
Recent HEAO 3 observations have been interpreted by Mahoney and colleagues as requiring approximately 3 M_sun; of 26Al alive in the interstellar medium. Calculations briefly discussed here indicate that there is substantial production and dispersal of 26Al in the stellar winds of O and W-R stars and suggest that the stellar winds of very massive stars are a significant source of 26Al.
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