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Parameterizing the Third Dredge up in AGB Stars
Published online by Cambridge University Press: 26 May 2016
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We present new evolutionary sequences for low and intermediate mass stars (1M⊙ to 6M⊙) for three different metallicities, z = 0.02, 0.008 and 0.004. We evolve the models from the pre-main sequence to the thermally-pulsing asymptotic giant branch (AGB) phase. We have two sequences of models for each mass, one which includes mass-loss and one without mass-loss. For an overview of AGB evolution and nucleosynthesis, see Herwig (2002) and Lattanzio (2002).
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- Part III: Planetary Nebulae in the Scheme of Stellar Evolution
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- Copyright © Astronomical Society of the Pacific 2003