Main Sequence Evolution
Main Sequence Evolution is a theoretical framework in stellar astrophysics that describes the phase of a star's life during which it fuses hydrogen into helium in its core, maintaining a stable structure determined by the balance between gravitational contraction and radiative pressure, thereby defining the dominant trajectory of stars on the Hertzsprung-Russell diagram.
779
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71K
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1.7K
Authors
593
Institutions
Publications per year
2017–2026
111
Parents
779
The Luminosity Function and Stellar Evolution.
E. E. Salpeter · The Astrophysical Journal · 1955 · 8.7K citations
Natural Sciences, Astronomy, Physics +16
Grids of stellar models with rotation
Sylvia Ekström, C. Georgy, P. Eggenberger et al. · Astronomy and Astrophysics · 2011 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
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593

Centre National de la Recherche Scientifique
Paris, France
40 h-index
159 publications
24.5K citations

Space Telescope Science Institute
Baltimore, United States
22 h-index
41 publications
4.6K citations
Osservatorio Astronomico di Padova
Padua, Italy
22 h-index
51 publications
5.2K citations
University of Geneva
Geneva, Switzerland
21 h-index
81 publications
25.6K citations
California Institute of Technology
Pasadena, United States
20 h-index
36 publications
2.5K citations
Université Paris Cité
Paris, France
19 h-index
46 publications
3.6K citations
Max Planck Institute for Astrophysics
Garching, Germany
18 h-index
30 publications
6K citations
European Southern Observatory
Santiago, Chile
16 h-index
36 publications
2K citations
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ApJ · 274 publications · 29.6K citations
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118 publications · 12.3K citations
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126 publications · 10.5K citations
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AJ · 43 publications · 2K citations
25
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18 publications · 3.8K citations
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