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- W2023851572 abstract "A model of supernova-driven chemical evolution of the Galactic halo proposed by Tsujimoto et al. ([CITE]) (TSY) is used to investigate the observations of the first generation stars (FGS). We assume in this paper that a star with a metallicity is truly a FGS. We obtain FGS probabilities with the Miller-Scalo form of the stellar initial mass function and limit our model parameters to values consistent with the observed metallicity distributions of metal-poor stars in the range of . We find a metallicity distribution function (MDF) of the long-lived halo field stars for against the iron abundance in agreement with the observations. If the star formation in the halo is confined to individual gas clouds with masses from 1 107 to , our model suggests that the probability of identifying FGS in the halo is about 6.14 10-5 to 6.14 10-6." @default.
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- W2023851572 date "2001-02-01" @default.
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- W2023851572 title "Research Note Prediction for the first generation stars from a Galactic halo chemical evolution model with Miller-Scalo initial mass function" @default.
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- W2023851572 doi "https://doi.org/10.1051/0004-6361:20000534" @default.
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