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• W2016088516 abstract "Nine silicon carbide grains of the rare type Z separated from the Murchison CM2 meteorite have been analyzed for the isotopic compositions of C, Si, N (seven grains), and Mg-Al (two grains) by ion microprobe mass spectrometry. These grains have 12C/13C ratios from 11 to 120,14N/15N ratios between 1100 and 19000, initial 26Al/27Al ratios of less than 0.003, and, relative to solar system Si, deficits in 29Si of up to 150 ‰ and enrichments in 30Si of up to 510 ‰. These isotopic signatures rule out the previously postulated nova or Type II supernova origin of the Z grains. Based on the predictions from a new asymptotic giant branch (AGB) star model it appears likely that the Z grains formed in the outflows of low-mass (<2.3 M☉), low-metallicity AGB stars that experienced strong cool bottom processing during the red giant phase." @default.
• W2016088516 created "2016-06-24" @default.
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• W2016088516 date "1997-09-20" @default.
• W2016088516 modified "2023-10-15" @default.
• W2016088516 title "Meteoritic Silicon Carbide Grains with Unusual S[CLC]i[/CLC]-Isotopic Compositions: Evidence for an Origin in Low-Mass, Low-Metallicity Asymptotic Giant Branch Stars" @default.
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• W2016088516 doi "https://doi.org/10.1086/310869" @default.
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