Nucleosynthesis Yields
Nucleosynthesis Yields is a theoretical construct in astrophysics that quantifies the total mass of each chemical element produced and ejected into the interstellar medium by a stellar population over its lifetime, distinguished by its role in modeling the chemical enrichment of galaxies.
355
Publications
40K
Citations
948
Authors
380
Institutions
Publications per year
2017–2026
83
Parents
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380

University of Minnesota
Minneapolis, United States
22 h-index
35 publications
5.3K citations
The University of Tokyo
Tokyo, Japan
19 h-index
51 publications
9.1K citations
Joint Institute for Nuclear Astrophysics
East Lansing, United States
19 h-index
62 publications
8.2K citations

Monash University
Melbourne, Australia
17 h-index
33 publications
4.8K citations
Los Alamos National Laboratory
Los Alamos, United States
17 h-index
87 publications
4.3K citations
Max Planck Institute for Astrophysics
Garching, Germany
16 h-index
41 publications
4.1K citations
GSI Helmholtz Centre for Heavy Ion Research
Darmstadt, Germany
16 h-index
24 publications
2.3K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
40 publications
2K citations
1–8 of 380
ApJ · 89 publications · 8.4K citations
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38 publications · 3.4K citations
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17 publications · 1.4K citations
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13 publications · 1.1K citations
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11 publications · 2.7K citations
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