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- W1609489651 abstract "Recent investigations of stellar chemical composition made it possible to estimate some parameters of the galactic disc chemical evolution: the abundance gradient, d[Fe/H]/dR, and rate of enrichment, d[Fe/H]/dt. Practically all the conclusions of these investigations were based on data on chemical composition of single stars, for which the error in age determination is considerable." @default.
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- W1609489651 date "1980-01-01" @default.
- W1609489651 modified "2023-09-25" @default.
- W1609489651 title "Rate of Enrichment of the Galactic Disc With Metals From Data on Open Clusters" @default.
- W1609489651 cites W1988650790 @default.
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- W1609489651 doi "https://doi.org/10.1017/s0074180900091701" @default.
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