Core Hydrogen Burning
Core Hydrogen Burning is a stellar energy-generation process, belonging to the class of nuclear fusion reactions, in which hydrogen nuclei are fused into helium in the central region of a star under high temperature and pressure, thereby distinguishing it from shell or non-central hydrogen burning phases.
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15.5K
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504
Authors
264
Institutions
Publications per year
2017–2026
37
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215
Bill Paxton, R. Smolec, Josiah Schwab et al. · The Astrophysical Journal Supplement Series · 2019 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
The Formation of Brown Dwarfs as Ejected Stellar Embryos
The Astronomical Journal · 2001 · 599 citations · Full text
Natural Sciences, Astronomy, Physics +12
U. Heber · Annual Review of Astronomy and Astrophysics · 2009 · 473 citations
Natural Sciences, Astronomy, Physics +17
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KU Leuven
Leuven, Belgium
13 h-index
28 publications
1.6K citations
Max Planck Institute for Astrophysics
Garching, Germany
11 h-index
11 publications
1.3K citations

Radboud University Nijmegen
Nijmegen, The Netherlands
9 h-index
14 publications
995 citations
University of Bonn
Bonn, Germany
9 h-index
35 publications
3.5K citations
Friedrich-Alexander-Universität Erlangen-Nürnberg
Erlangen, Germany
9 h-index
31 publications
1.5K citations
University of Geneva
Geneva, Switzerland
8 h-index
21 publications
900 citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
20 publications
991 citations
Universitat Politècnica de Catalunya
Barcelona, Spain
7 h-index
11 publications
1.4K citations
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ApJ · 77 publications · 5.7K citations
38
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41 publications · 2.6K citations
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28 publications · 1.1K citations
18
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7 publications · 440 citations
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AJ · 7 publications · 718 citations
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