Stellar Nucleosynthesis
Stellar Nucleosynthesis is an astrophysical process of nucleosynthesis in which chemical elements are formed and transmuted through nuclear fusion and associated nuclear reactions in the interiors and explosive endpoints of stars, thereby producing most elements heavier than those created in Big Bang nucleosynthesis.
2.2K
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2017–2026
426
2.2K
Synthesis of the Elements in Stars
E. M. Burbidge, G. R. Burbidge, William A. Fowler et al. · Reviews of Modern Physics · 1957 · 4K citations · Full text
Nucleosynthesis, neutrino bursts and γ-rays from coalescing neutron stars
David Eichler, Mario Livio, Tsvi Piran et al. · Nature · 1989 · 2.1K citations
Natural Sciences, Astronomy, Physics +12
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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The University of Tokyo
Tokyo, Japan
71 h-index
317 publications
40.9K citations
Max Planck Institute for Astrophysics
Garching, Germany
65 h-index
205 publications
35.2K citations
Joint Institute for Nuclear Astrophysics
East Lansing, United States
58 h-index
335 publications
26.5K citations

University of Basel
Basel, Switzerland
57 h-index
200 publications
28.2K citations
Michigan State University
East Lansing, United States
56 h-index
197 publications
15.2K citations

Monash University
Melbourne, Australia
55 h-index
207 publications
19.7K citations

Centre National de la Recherche Scientifique
Paris, France
53 h-index
265 publications
23.1K citations
University of Chicago
Chicago, United States
52 h-index
181 publications
18.5K citations
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ApJ · 751 publications · 75.2K citations
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183 publications · 14.3K citations
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177 publications · 15.1K citations
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