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• W2157577462 startingPage "549" @default.
• W2157577462 abstract "The local thermodynamic equilibrium (LTE) abundances of zinc (Zn) of our sample of 35 metal-poor stars were explored in the range of |$-$|3.0 |$<$| [Fe|$/$|H] |$<$| 0.0. Based on a combination of our Zn abundances and those obtained in the literature, the behavior of Zn was investigated in the range of |$-$|4.2 |$<$| [Fe|$/$|H] |$<$||$+$|0.5. The main results are as follows: (1) No clear separation in [Zn|$/$|Fe] behavior was found between halo, thick disk, and thin disk stars in our sample. (2) The decreasing trend of [Zn|$/$|Fe] with the increase of [Fe|$/$|H] was found to be confirmed to |$-$|4.2 |$<$| [Fe|$/$|H] |$le$||$-$|2.0, and to be explained by a chemical evolution model constructed with models of core-collapse supernovae (SNe) II or hypernovae (HNe) of Population III stars. (3) In |$-$|2.0 |$<$| [Fe|$/$|H] |$<$||$+$|0.5, [Zn|$/$|Fe] follows a nearly flat trend with a slight enhancement of |$sim+$|0.07 dex up to [Fe|$/$|H] |$=$||$-$|1.0, and shows the more enhanced trend in |$-$|1.0 |$<$| [Fe|$/$|H] |$le$||$-$|0.5, and then gradually decreases to an almost solar value in [Fe|$/$|H] |$>$||$-$|0.5. This trend is better explained by a chemical evolution model constructed with models of normal SNe II, HNe, and SNe Ia, in which the metallicity effect and the single-degenerate scenario of the SNe Ia model are incorporated." @default.
• W2157577462 created "2016-06-24" @default.
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• W2157577462 date "2009-06-25" @default.
• W2157577462 modified "2023-09-26" @default.
• W2157577462 title "Chemical Evolution of Zinc in the Galaxy" @default.
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• W2157577462 doi "https://doi.org/10.1093/pasj/61.3.549" @default.
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