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Galacti chemical evolution: Hygrogen through zinc

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Timmes, F. X., Woosley, S. E., Weaver, Thomas A.·1995·The Astrophysical Journal Supplement Series

Abstract

Using the output from a grid of 60 Type II supernova models (Woosley \& Weaver 1994) of varying mass (11 $\ltaprx$ M/M\sun $\ltaprx$ 40) and metallicity (0, 10$^{-4}$, 0.01, 0.1, and 1 Z\sol), the chemical evolution of 76 stable isotopes, from hydrogen to zinc, is calculated. The chemical evolution calculation employs a simple dynamical model for the Galaxy (infall with a 4 billion year $e$-folding time scale onto a exponential disk and 1/r$^2$ bulge), and standard evolution parameters, such as a Salpeter initial mass function and a quadratic Schmidt star formation rate. The theoretical results are compared in detail with observed stellar abundances in stars with metallicities in the range -3.0 $\ltaprx$ [Fe/H] $\ltaprx$ 0.0 dex. While our discussion focuses on the solar neighborhood where there are the most observations, the supernovae rates, an intrinsically Galactic quantity, are also discussed.

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Metadata

Authors
Timmes, F. X., Woosley, S. E., & Weaver, T. A.
Venue
The Astrophysical Journal Supplement Series
Published
1995-06
Volume
98
Pages
617
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W1639491943
Cited by
900
References
0
Type
conference abstract
Language
en
Open access
green

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CoChat. (2026). Citation check: Galacti chemical evolution: Hygrogen through zinc. https://app.cochat.ai/papers/10.1086/192172
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Timmes, F. X., Woosley, S. E., & Weaver, T. A. (1995). Galacti chemical evolution: Hygrogen through zinc. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/192172

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