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- W2029263067 abstract "We present a new chemical evolution model for the Galaxy that assumes two main infall episodes, for the formation of the halo-thick disk and thin disk, respectively. We do not try to take into account explicitly the evolution of the halo since our model is better suited for computing the evolution of the disk (thick plus thin), but we implicitly assume that the timescale for the formation of the halo was of the same order as the timescale for the formation of the thick disk. The formation of the thin disk is much longer than that of the thick disk, implying that the infalling gas forming the thin disk comes not only from the thick disk but mainly from the intergalactic medium." @default.
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- W2029263067 date "1997-03-10" @default.
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- W2029263067 title "The Chemical Evolution of the Galaxy: The Two‐Infall Model" @default.
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- W2029263067 doi "https://doi.org/10.1086/303726" @default.
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