Elemental Nucleosynthesis
Elemental Nucleosynthesis is a theoretical framework in astrophysics that describes the process by which new atomic nuclei are formed through nuclear fusion reactions in the extreme conditions following a supernova explosion, distinguishing it from primordial and stellar nucleosynthesis by its reliance on explosive nucleosynthetic pathways and shock-induced reactions.
948
Publications
88.7K
Citations
2.2K
Authors
745
Institutions
Publications per year
2017–2026
179
Parents
948
A grid of MARCS model atmospheres for late-type stars
B. Gustafsson, B. Edvardsson, Kimmo Eriksson et al. · Astronomy and Astrophysics · 2008 · 2.6K citations · Full text
The Nucleosynthetic Signature of Population III
Alexander Heger, S. E. Woosley · The Astrophysical Journal · 2002 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
Koichi Iwamoto, F. Brachwitz, Ken’ichi Nomoto et al. · The Astrophysical Journal Supplement Series · 1999 · 1.4K citations · Full text
Natural Sciences, Astronomy, Physics +16
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745
The University of Tokyo
Tokyo, Japan
43 h-index
146 publications
18.8K citations
Max Planck Institute for Astrophysics
Garching, Germany
34 h-index
93 publications
12.8K citations
California Institute of Technology
Pasadena, United States
33 h-index
110 publications
9.7K citations
Joint Institute for Nuclear Astrophysics
East Lansing, United States
32 h-index
134 publications
10.4K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
31 h-index
80 publications
8.1K citations

Monash University
Melbourne, Australia
30 h-index
73 publications
8.5K citations

University of Basel
Basel, Switzerland
30 h-index
75 publications
9K citations
Michigan State University
East Lansing, United States
30 h-index
88 publications
5.8K citations
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ApJ · 296 publications · 29.6K citations
86
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75 publications · 7.9K citations
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65 publications · 4.8K citations
35
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27 publications · 2.6K citations
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27 publications · 2K citations
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