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- W1997372632 abstract "The basic equations for chemical evolution, allowing radial flow of gas in two- and three-dimensional galaxies, are examined, and a few general constraints are derived. A formalism is developed for the evolution of chemical abundances with radial flows, no accretion, and fairly general Schmidt-type star formation laws. Quantities of observational interest (such as gas density, gas chemical abundance, mean stellar metal abundance and star density) may be expressed as a function of galactic radius either as analytic functions or, at worst, as straightforward integrals. By investigating a few particularly simple cases in detail, we demonstrate the general effects of radial flows on the chemical evolution of galaxies and abundance gradients." @default.
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- W1997372632 date "1995-01-01" @default.
- W1997372632 modified "2023-10-16" @default.
- W1997372632 title "General constraints on the effect of gas flows in the chemical evolution of galaxies - II. Radial flows and abundance gradients" @default.
- W1997372632 doi "https://doi.org/10.1093/mnras/272.2.241" @default.
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