Shell Burning
Shell Burning is a nuclear fusion process in stellar interiors wherein fusion reactions occur in a concentric layer surrounding a degenerate core, distinguished from core burning by its spatial confinement to a shell-like region where temperature and pressure conditions enable the ignition of heavier elements.
101
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6.6K
Citations
264
Authors
169
Institutions
Publications per year
2017–2026
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169
The University of Tokyo
Tokyo, Japan
11 h-index
18 publications
1.1K citations
University of Arizona
Tucson, United States
10 h-index
17 publications
1.1K citations
Los Alamos National Laboratory
Los Alamos, United States
6 h-index
6 publications
649 citations

Monash University
Melbourne, Australia
6 h-index
12 publications
1.1K citations
Max Planck Institute for Astrophysics
Garching, Germany
5 h-index
12 publications
1.4K citations
Michigan State University
East Lansing, United States
4 h-index
5 publications
781 citations

Keio University
Tokyo, Japan
4 h-index
4 publications
391 citations
Queen's University Belfast
Belfast, United Kingdom
4 h-index
6 publications
573 citations
1–8 of 169
ApJ · 43 publications · 3.1K citations
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14 publications · 630 citations
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5 publications · 158 citations
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PASP · 4 publications · 389 citations
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3 publications · 69 citations
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