Explosive nucleosynthesis revisited: Yields

David Arnett

doi:10.1146/annurev.aa.33.090195.000555

Explosive nucleosynthesis revisited: Yields

David Arnett

Research output: Contribution to journal › Article › peer-review

38 Scopus citations

Abstract

Three new, independent projects that provide detailed predictions of nucleosynthesis yields (up to Z = 36) from massive stars are examined and compared. The general agreement is surprisingly good. Preliminary comparison with abundance data, especially for elemental abundances in extreme Population II stars, is promising. Implications of these comparisons and critical uncertainties are discussed.

Original language	English (US)
Pages (from-to)	115-132
Number of pages	18
Journal	Annual Review of Astronomy and Astrophysics
Volume	33
Issue number	1
DOIs	https://doi.org/10.1146/annurev.aa.33.090195.000555
State	Published - 1995
Externally published	Yes

Keywords

Abundances
Big Bang
Galactic evolution
Population II
Stars
Supernovae

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1146/annurev.aa.33.090195.000555

Cite this

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title = "Explosive nucleosynthesis revisited: Yields",

abstract = "Three new, independent projects that provide detailed predictions of nucleosynthesis yields (up to Z = 36) from massive stars are examined and compared. The general agreement is surprisingly good. Preliminary comparison with abundance data, especially for elemental abundances in extreme Population II stars, is promising. Implications of these comparisons and critical uncertainties are discussed.",

keywords = "Abundances, Big Bang, Galactic evolution, Population II, Stars, Supernovae",

author = "David Arnett",

year = "1995",

doi = "10.1146/annurev.aa.33.090195.000555",

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AB - Three new, independent projects that provide detailed predictions of nucleosynthesis yields (up to Z = 36) from massive stars are examined and compared. The general agreement is surprisingly good. Preliminary comparison with abundance data, especially for elemental abundances in extreme Population II stars, is promising. Implications of these comparisons and critical uncertainties are discussed.

KW - Abundances

KW - Big Bang

KW - Galactic evolution

KW - Population II

KW - Stars

KW - Supernovae

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ER -

Explosive nucleosynthesis revisited: Yields

Abstract

Keywords

ASJC Scopus subject areas

Access to Document

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