Fig. C.2
Ejection rates of hydrogen, carbon, oxygen and Fe from a stellar population of 1 M⊙ as a function of time. Yields are from Nomoto et al. (2013).The curves represent different metallicities, as indicated in the top panel. The dotted curves show the contribution of SNIa (resulting from a SSP of 1 M⊙) to the production of those elements.
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