Pre-main-sequence Stellar Evolution
Pre-Main-Sequence Stellar Evolution is a theoretical construct in astrophysics denoting the phase of stellar development from gravitational collapse of a molecular cloud core to the onset of stable hydrogen fusion on the main sequence, distinguished by energy generation primarily through gravitational contraction and accretion rather than core nuclear fusion.
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Pms Stellar Evolution
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MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
Jieun Choi, Aaron Dotter, Charlie Conroy et al. · The Astrophysical Journal · 2016 · 2.8K citations · Full text
Natural Sciences, Astronomy, Physics +14
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Centre National de la Recherche Scientifique
Paris, France
29 h-index
98 publications
8.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
21 h-index
42 publications
11.1K citations
University of Vienna
Vienna, Austria
15 h-index
27 publications
2.5K citations
University of Geneva
Geneva, Switzerland
15 h-index
54 publications
3.1K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
14 h-index
36 publications
2.2K citations
Institute of Astronomy
Moscow, Russia
14 h-index
24 publications
2K citations
The University of Tokyo
Tokyo, Japan
14 h-index
39 publications
4.3K citations
The University of Texas at Austin
Austin, United States
13 h-index
24 publications
2.2K citations
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ApJ · 130 publications · 17.3K citations
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AJ · 28 publications · 1.3K citations
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