Very massive star winds as sources of the short-lived radioactive isotope Al-26
Context. The Al-26 short-lived radioactive nuclide is the source of the observed galactic diffuse gamma-ray emission at 1.8 MeV. While different sources of Al-26 have been explored, such as asymptotic giant branch stars, massive stellar winds, and supernovae, the contribution of very massive stars h...
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Main Authors: | Martinet, Sebastien, Meynet, Georges, Nandal, Devesh, Ekstrom, Sylvia, Georgy, Cyril, Haemmerle, Lionel, Hirschi, Raphael, Yusof, Norhasliza, Gounelle, Matthieu, Dwarkadas, Vikram |
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Format: | Article |
Published: |
EDP Sciences S A
2022
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Online Access: | http://eprints.um.edu.my/41335/ |
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