The Chemical Yields Produced by Zero Metal Massive Stars

Preprint

31 May 2002

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/0205543

Abstract

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 38245. 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

METAL MASSIVE STARS
ZERO METAL MASSIVE
YIELDS PRODUCED
CHEMICAL YIELDS
THEORETICAL SET
SETS OF YIELDS

All Related Versions

Version 1, 2002-05-31, ArXiv
Published version: Publications of the Astronomical Society of Australia, 19 (2), 246.

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