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- W52941285 abstract "To the aim of reproducing the oxygen abundances and gradients observed in the disk of our Galaxy and four nearby spirals (M31, M33, M83, and M101), we have computed numerical models of galactic evolution assuming only two free parameters: the infall of gas from outside the disk and the law of star formation (e.g. proportional to some power of the gas density, decreasing with time, constant, etc.)." @default.
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- W52941285 date "1984-01-01" @default.
- W52941285 modified "2023-09-26" @default.
- W52941285 title "Theoretical predictions for the radial distribution of oxygen in spiral galaxies" @default.
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- W52941285 doi "https://doi.org/10.1017/s0074180900031478" @default.
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