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• W2023240653 abstract "I evaluate several nuclear and chemical problems related both to the recent scenario suggesting that the known isotopic anomalies in the solar system have resulted from a supernova near the protosolar nebula and to the model of extinct presolar carriers. Major features include: (1) Large quantities of extinct 248Cm and 36Cl are predicted from the Cameron-Truran model of a minor injection about 106 yr before condensation; (2) an extinct-carrier model of 26Mg is set forth in detail with a solid chemistry picture of the early solar system; (3) a major thermonuclear supernova responsible for 26Al, 244Pu, and 40K would have to have occurred several million years (3 m.y.) before condensation and contributed a large fraction of the major stable chemical elements; (4) carbon isotope families are to be expected if the oxygen isotope families are due to a late injection of 16O; (5) the Earth and E meteorites may have condensed primarily in a carbon-rich nebula existing before admixtures of a major late 16O-rich mixture; (6) the extinct-presolar-carrier model is the single best explanation of all anomalies." @default.
• W2023240653 created "2016-06-24" @default.
• W2023240653 creator A5008871798 @default.
• W2023240653 date "1977-11-01" @default.
• W2023240653 modified "2023-10-14" @default.
• W2023240653 title "Solar system isotopic anomalies: Supernova neighbor or presolar carriers?" @default.
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• W2023240653 doi "https://doi.org/10.1016/0019-1035(77)90001-x" @default.
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