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Please use this identifier to cite or link to this item: http://hdl.handle.net/10481/29052

Title: The role of gravitational supernovae in the Galactic evolution of the Li, Be and B isotopes
Authors: Abia, Carlos
Isern, Jordi
Lisenfeld, Ute
Issue Date: 1998
Abstract: The observed Be and B relationships with metallicity clearly support the idea that both elements have a primary origin and that are produced by the same class of objects. Spallation by particles accelerated during gravitational events (SNII, SNIb/c) seems to be a likely origin. We show, in the context of a model of chemical evolution, that it is possible to solve the Li, Be and B abundance puzzle with the yields recently proposed by Ramaty et al. (1997), provided that SNII are unable to significantly accelerate helium nuclei and that different mechanisms are allowed to act simultaneously.
Publisher: Oxford University Press (OUP); Royal Astronomical Society
Keywords: Nuclear reactions
Nucleosynthesis
Abundances
Supernovae
Galaxy
URI: http://hdl.handle.net/10481/29052
ISSN: 0035-8711
1365-2966
Rights : Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License
Citation: Abia, C.; Isern, J.; Lisenfeld, U. The role of gravitational supernovae in the Galactic evolution of the Li, Be and B isotopes. Monthly Notices of the Royal Astronomical Society, 299(4): 1007-1012. [http://hdl.handle.net/10481/29052]
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