The role of low metallicity AGB stars in globular cluster evolution

Details The role of low metallicity AGB stars in globular cluster evolution The role of low metallicity AGB stars in globular cluster evolution

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..283d&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Physics

Scientific paper

We compute models of intermediate mass stars from the pre-main sequence up to the end of the thermal pulse phase on the asymptotic giant branch with the code STAREVOL. Models of 6 solar masses are presented for two metallicities which correspond respectively to the metallicity of the LMC and of the most metal-poor globular clusters (Z=0.008 and 0.0001). These models include the most up-to-date input physics (nuclear reactions, eos, mass loss, ...). We focus on the the nucleosynthesis that occurs in these objects and on the corresponding stellar yields.

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