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- W4302789584 abstract "In the relatively gas-rich, pure exponential disk galaxies, available data is accumulating which suggests that the distribution of starformation in the disk either shows no radial variation, or else has a scale-length which is much longer than that of the stars." @default.
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- W4302789584 date "1987-01-01" @default.
- W4302789584 modified "2023-09-26" @default.
- W4302789584 title "Disk Galaxies: The Global Properties of Star Formation and the Chemical Abundance Gradients" @default.
- W4302789584 doi "https://doi.org/10.1017/s0074180900096546" @default.
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