Stellar Models and Yields of Asymptotic Giant Branch Stars release_schr73zxozfzzk3j2ecbgluyku

by Amanda I. Karakas, John C. Lattanzio

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abstracts[] {'sha1': '00f63bccac13a185359f541eabd3914b6f9aa65d', 'content': 'We present stellar yields calculated from detailed models of low and\nintermediate-mass asymptotic giant branch (AGB) stars. We evolve models with a\nrange of mass from 1 to 6Msun, and initial metallicities from solar to 1/200th\nof the solar metallicity. Each model was evolved from the zero age main\nsequence to near the end of the thermally-pulsing AGB phase, and through all\nintermediate phases including the core He-flash for stars initially less\nmassive than 2.5Msun. For each mass and metallicity, we provide tables\ncontaining structural details of the stellar models during the TP-AGB phase,\nand tables of the stellar yields for 74 species from hydrogen through to\nsulphur, and for a small number of iron-group nuclei. All tables are available\nfor download. Our results have many applications including use in population\nsynthesis studies and the chemical evolution of galaxies and stellar systems,\nand for comparison to the composition of AGB and post-AGB stars and planetary\nnebulae.', 'mimetype': 'text/plain', 'lang': 'en'}
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{'index': 1, 'creator_id': None, 'creator': None, 'raw_name': 'John C. Lattanzio', 'given_name': None, 'surname': None, 'role': 'author', 'raw_affiliation': None, 'extra': None}
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release_date 2007-10-10
release_stage accepted
release_type article
release_year 2007
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title Stellar Models and Yields of Asymptotic Giant Branch Stars
version v2
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arxiv.base_id 0708.4385
arxiv.categories ['astro-ph']
arxiv.comments 26 pages; to appear in Publications of the Astronomical Society of Australia (PASA); typos fixed in the text and in Tables 4 and 6
arxiv.journal_ref Publ.Astron.Soc.Austral.24:103-117,2007