Shell Hydrogen Burning is a stellar nucleosynthesis process in which hydrogen fuses into helium in a concentric layer surrounding the inert core of a red giant star, driven by gravitational contraction and distinct from core hydrogen burning in main-sequence stars.
122
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267
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141
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2017–2026
13
Parents
Publications
122
The evolution and fate of Very Massive Objects
J. Richard Bond, W. David Arnett, B. J. Carr · The Astrophysical Journal · 1984 · 407 citations
Natural Sciences, Astronomy, Physics +17
Very low-metallicity massive stars:
Raphaël Hirschi · Astronomy and Astrophysics · 2006 · 253 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 122
Authors
267
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7
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7
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4
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3
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1–5 of 267
Institutions
141
Collurania Teramo Observatory
Teramo, Italy
9 h-index
13 publications
476 citations
Yale University
New Haven, United States
7 h-index
11 publications
349 citations
The University of Tokyo
Tokyo, Japan
6 h-index
9 publications
852 citations
Monash University
Melbourne, Australia
5 h-index
10 publications
1.3K citations
Keio University
Tokyo, Japan
5 h-index
5 publications
509 citations
Liverpool John Moores University
Liverpool, United Kingdom
4 h-index
4 publications
116 citations
University of Victoria
Victoria, Canada
4 h-index
8 publications
275 citations
University of California, Santa Cruz
Santa Cruz, United States
4 h-index
6 publications
359 citations
1–8 of 141
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- The Astrophysical Journal
ApJ · 58 publications · 4K citations
32
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- Monthly Notices of the Royal Astronomical Society
18 publications · 848 citations
15
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- Astronomy and Astrophysics
12 publications · 974 citations
12
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- CERN Document Server (European Organization for Nuclear Research)
Repository · 4 publications · 74 citations
4
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- The Astrophysical Journal Supplement Series
3 publications · 329 citations
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