Pre-Main-Sequence Rotation is a stellar rotational phenomenon characterized by the angular momentum evolution of young, contracting stars prior to their arrival on the main sequence, distinguished from main-sequence rotation by its dependence on accretion processes, disk interactions, and non-homologous contraction during early evolutionary phases.
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ROTATION IN THE PLEIADES WITH K2. I. DATA AND FIRST RESULTS
The Astronomical Journal · 2016 · 215 citations · Full text
Natural Sciences, Astronomy, Physics +12
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Centre National de la Recherche Scientifique
Paris, France
20 h-index
47 publications
3.3K citations
University of Geneva
Geneva, Switzerland
14 h-index
38 publications
2.5K citations
Université Grenoble Alpes
Saint-Martin-d'Hères, France
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16 publications
1.4K citations
California Institute of Technology
Pasadena, United States
11 h-index
27 publications
3K citations
Ames Research Center
Mountain View, United States
10 h-index
11 publications
962 citations
University of Exeter
Exeter, United Kingdom
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16 publications
487 citations
University of St Andrews
St Andrews, United Kingdom
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990 citations
Université Fédérale de Toulouse Midi-Pyrénées
Toulouse, France
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ApJ · 46 publications · 2.8K citations
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Repository · 4 publications · 118 citations
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