Galactic Chemical Evolution
Galactic Chemical Evolution is a theoretical framework in astrophysics that describes the progressive change in chemical composition of baryonic matter within galaxies over cosmic time due to stellar nucleosynthesis, supernova explosions, and galactic-scale gas dynamics.
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Citations
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790
Institutions
Publications per year
2017–2026
278
1.3K
The Geneva-Copenhagen survey of the Solar neighbourhood
B. Nordström, M. Mayor, J. Andersen et al. · Astronomy and Astrophysics · 2004 · 1.6K citations · Full text
Natural Sciences, Astronomy, Physics +16
Compositions of halo clusters and the formation of the galactic halo
Leonard Searle, R. Zinn · The Astrophysical Journal · 1978 · 1.5K citations
Natural Sciences, Astronomy, Physics +17
The Chemical Evolution of the Galaxy: The Two‐Infall Model
C. Chiappini, F. Matteuccí, R. Gratton · The Astrophysical Journal · 1997 · 941 citations · Full text
Natural Sciences, Astronomy, Physics +17
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790

Centre National de la Recherche Scientifique
Paris, France
56 h-index
385 publications
36.4K citations

Trieste Astronomical Observatory
Trieste, Italy
52 h-index
215 publications
15K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
45 h-index
131 publications
17.5K citations
University of Cambridge
Cambridge, United Kingdom
39 h-index
117 publications
14.8K citations
The University of Tokyo
Tokyo, Japan
38 h-index
118 publications
27.3K citations

Australian National University
Canberra, Australia
38 h-index
88 publications
7.9K citations
Institut d'Astrophysique de Paris
Paris, France
37 h-index
83 publications
11.5K citations
National Institute for Astrophysics
Rome, Italy
36 h-index
87 publications
8.1K citations
1–8 of 790
ApJ · 379 publications · 38.9K citations
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227 publications · 17.8K citations
71
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211 publications · 15.8K citations
68
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AJ · 44 publications · 3.7K citations
28
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Repository · 43 publications · 1.7K citations
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