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Low-Mass AGB Stellar Models for 0.003 ≤ Z ≤ 0.02: Basic Formulae for Nucleosynthesis Calculations

Published online by Cambridge University Press:  05 March 2013

O. Straniero ,
I. Domínguez ,
S. Cristallo  and
R. Gallino
O. Straniero
Affiliation:
INAF, Osservatorio Astronomico di Teramo, Italystraniero@te.astro.it
I. Domínguez
Affiliation:
Universidad de Granada, Spaininma@ugr.es
S. Cristallo
Affiliation:
INAF, Osservatorio Astronomico di Teramo, Italycristallo@te.astro.it
R. Gallino
Affiliation:
Dip. Fisica Generale Università di Torino and Sez. INFN Torino, Italygallino@ph.unito.it Center for Stellar and Planetary Astrophysics, Monash University, Melbourne 3800, Australia
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Abstract

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We have extended our published set of low-mass AGB stellar modelsto lower metallicities. Different mass-loss rates have been explored. We provide interpolation formulae for the luminosity, effective temperature, core mass, mass of dredge up material and maximum temperature in the convective zone generated by thermal pulses. Finally, we discuss the resultant modification of these quantities when we use an appropriate treatment of the inward propagation of the convective instability, as caused by the steeprise in radiative opacity when the convective envelope penetratesthe H-depleted region.

Keywords

stars: abundancesstars: AGBstars: evolutionnucleosynthesis
Type
Sixth Torino Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 4 , 2003 , pp. 389 - 392
Copyright
Copyright © Astronomical Society of Australia 2003

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