Implications from inhomogeneous chemical evolution: Yields of O-Zn

Details Implications from inhomogeneous chemical evolution: Yields of O-Zn Implications from inhomogeneous chemical evolution: Yields of O-Zn

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..671i&link_type=abstract

Nuclear Physics A, Volume 718, p. 671-673.

Physics

Nuclear Physics

4

Scientific paper

Observations of metal-poor stars show intrinsic large dispersions in their chemical abundances. This may indicate that these stars are enriched by only one or a few supernovae, since the inter-stellar gas was not mixed enough at the early epoch. We construct an inhomogeneous chemical evolution model, and compare predicted stellar abundance distributions for O-Zn with observations. Using statistical method, we show clear differences between two sets of yields; by and by .

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