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The Chemical Yields Produced by Zero Metal Massive Stars*

Published online by Cambridge University Press:  05 March 2013

Marco Limongi  and
Alessandro Chieffi
Marco Limongi
Affiliation:
Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio Catone (Roma), Italy, I-00040; marco@mporzio.astro.it
Alessandro Chieffi
Affiliation:
Osservatorio Astronomico di Roma, Via Frascati 33, Monteporzio Catone (Roma), Italy, I-00040 Istituto di Astrofisica Spaziale (CNR), Via Fosso del Cavaliere, Roma, Italy, I-00133; achieffi@ias.rm.cnr.it
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Abstract

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In this review we compare the three existing sets of theoretical yields of zero metal massive stars available in the literature. We also show how each of these three different sets of yields fits the element abundance ratios observed in the extremely metal poor star CD 38°245. We find that, at present, no theoretical set of yields of zero metal massive stars is able to satisfactorily reproduce the elemental ratios [X/Fe] of this star.

Keywords

stars: evolutionnucleosynthesissupernovae: generalstars: abundancesGalaxy: formation
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 19 , Issue 2 , 2002 , pp. 246 - 256
Copyright
Copyright © Astronomical Society of Australia 2002

Footnotes

*

Invited Talk, Annual Conference of the Astronomical Society of Australia, Lorne, 2–4 July, 2001.

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