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- W1968658045 abstract "We calculated the evolution of surface heavy elements and CO ratio for a 3 M⊙ thermal-pulse, AGB star with initial metallicity 0.015, based on the theories of the s-process and star evolution. For reasonable parameter values, our calculated curve falls within the observed regions of the MS, S and C stars in the abundance and CO diagrams. The range of the neutron irradiance is τ0 = 0.2–0.6 mb−1. Under the reasonable assumption that dredge-up occurs after the asymptotic distribution is established, factors such as whether or not the core mass or the mass dredged-up varies with the pulse number have little effect on the surface abundance of intrinsic AGB stars. The dredge-up-starting pulse number affects the abundance of MS and S stars more than that of the C stars." @default.
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- W1968658045 date "1998-01-01" @default.
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- W1968658045 title "Evolution of the surface abundance of a 3 M⊙ AGB star" @default.
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- W1968658045 doi "https://doi.org/10.1016/s0275-1062(98)00007-1" @default.
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