Supernova Yields
Supernova Yields is a theoretical construct in astrophysics that quantifies the mass of newly synthesized elements ejected into the interstellar medium by a supernova explosion, distinguishing it from other nucleosynthetic outputs through its specific association with explosive stellar death.
169
Publications
14.9K
Citations
374
Authors
230
Institutions
Publications per year
2017–2026
44
Parents
169
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
R. Cayrel, É. Depagne, M. Spite et al. · Astronomy and Astrophysics · 2004 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +11
Galactic Chemical Evolution: Carbon through Zinc
Chiaki Kobayashi, Hideyuki Umeda, K. Nomoto et al. · The Astrophysical Journal · 2006 · 877 citations · Full text
NUCLEOSYNTHESIS AND EVOLUTION OF MASSIVE METAL-FREE STARS
Alexander Heger, S. E. Woosley · The Astrophysical Journal · 2010 · 700 citations · Full text
Natural Sciences, Astronomy, Physics +17
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230
The University of Tokyo
Tokyo, Japan
21 h-index
49 publications
9.8K citations
Joint Institute for Nuclear Astrophysics
East Lansing, United States
18 h-index
50 publications
2.5K citations

Monash University
Melbourne, Australia
14 h-index
20 publications
2.4K citations
Los Alamos National Laboratory
Los Alamos, United States
12 h-index
31 publications
2.2K citations
Michigan State University
East Lansing, United States
11 h-index
16 publications
1.8K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
11 h-index
13 publications
2.3K citations
Max Planck Institute for Astrophysics
Garching, Germany
10 h-index
24 publications
3.6K citations

University of Minnesota
Minneapolis, United States
10 h-index
15 publications
1.4K citations
1–8 of 230
ApJ · 66 publications · 6.7K citations
38
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24 publications · 1.7K citations
20
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16 publications · 2.1K citations
16
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Repository · 5 publications · 387 citations
5
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4 publications · 433 citations
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