Pre-main-sequence Evolution
Pre-Main-Sequence Evolution is the phase of stellar evolution wherein a protostar contracts gravitationally and accretes mass prior to reaching the main sequence, distinguished from subsequent evolutionary stages by the absence of sustained hydrogen fusion in its core.
420
Publications
37.4K
Citations
792
Authors
394
Institutions
Publications per year
2017–2026
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Centre National de la Recherche Scientifique
Paris, France
30 h-index
78 publications
17.1K citations
University of Geneva
Geneva, Switzerland
25 h-index
122 publications
7.8K citations
The University of Tokyo
Tokyo, Japan
16 h-index
28 publications
2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
32 publications
1.7K citations
National Institute for Astrophysics
Rome, Italy
14 h-index
25 publications
1.9K citations

Keele University
Newcastle-under-Lyme, United Kingdom
14 h-index
22 publications
2.7K citations
Arcetri Astrophysical Observatory
Florence, Italy
13 h-index
20 publications
2.2K citations
California Institute of Technology
Pasadena, United States
13 h-index
21 publications
2.4K citations
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ApJ · 117 publications · 11.8K citations
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77 publications · 6.7K citations
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62 publications · 6.3K citations
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AJ · 20 publications · 1.3K citations
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Repository · 13 publications · 1.8K citations
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