THE PRODUCTION AND DEPLETION RATES IN MODELS
FOR THE CHEMICAL EVOLUTION OF THE GALAXY
L. I. Arany-Prado, W. J. Maciel
Rev. Mexicana Astron. Astrophys. 34, 21-28 (1998)
The stellar production and depletion rates associated with a given metal are
derived, to be used in the general equation for the mass conservation in
models of the chemical evolution of the Galaxy. It is shown that the metal
conservation equation of Tinsley (1980) can be recovered with the adoption
of some simplifying hypotheses, such as neglecting the metals
stored in the remnants. With the derived equation, we show that the total
mass of a given metal can be affected by the hypotheses usually made.
For the bulk of metals, we find that their total mass can be increased
up to an order of magnitude relative to the expected mass of metals as
given by Tinsley (1980).
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