Stellar Evolutionary Models
Stellar Evolutionary Models is a theoretical framework that describes the physical processes and structural changes governing the life cycle of stars from their formation in molecular clouds through the main sequence, with particular emphasis on pre-main-sequence contraction, accretion, and energy transport mechanisms distinguishing it from post-main-sequence evolutionary theories.
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2017–2026
455
Variants
Stellar Evolution Models
Parents
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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
71 h-index
628 publications
74.5K citations

Space Telescope Science Institute
Baltimore, United States
56 h-index
206 publications
19.5K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
53 h-index
172 publications
27.5K citations
Osservatorio Astronomico di Padova
Padua, Italy
51 h-index
241 publications
65.3K citations
University of Geneva
Geneva, Switzerland
48 h-index
306 publications
47.1K citations
Max Planck Institute for Astrophysics
Garching, Germany
47 h-index
160 publications
42.8K citations
Collurania Teramo Observatory
Teramo, Italy
43 h-index
99 publications
12.2K citations
Université Paris Cité
Paris, France
43 h-index
143 publications
9.8K citations
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ApJ · 916 publications · 90.4K citations
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493 publications · 39.7K citations
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406 publications · 48.1K citations
90
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73 publications · 19.1K citations
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AJ · 99 publications · 5.6K citations
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