Main-sequence Stars
Main-Sequence Stars is a class of stars in stellar astrophysics that are in the long-lived, hydrostatic-equilibrium phase of their evolution during which they generate energy primarily by fusing hydrogen into helium in their cores and consequently occupy the main sequence locus in the Hertzsprung–Russell diagram.
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The Luminosity Function and Stellar Evolution.
E. E. Salpeter · The Astrophysical Journal · 1955 · 8.7K citations
Natural Sciences, Astronomy, Physics +16
Habitable Zones around Main Sequence Stars
James F. Kasting, D. P. Whitmire, R. T. Reynolds · Icarus · 1993 · 2.5K citations
Natural Sciences, Astronomy, Physics +14
Rotation, convection, and magnetic activity in lower main-sequence stars
R. W. Noyes, Lee Hartmann, S. L. Baliunas et al. · The Astrophysical Journal · 1984 · 1.8K citations
Natural Sciences, Astronomy, Physics +14
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Centre National de la Recherche Scientifique
Paris, France
59 h-index
380 publications
34.8K citations
California Institute of Technology
Pasadena, United States
44 h-index
143 publications
12.8K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
43 h-index
138 publications
12.6K citations

Space Telescope Science Institute
Baltimore, United States
40 h-index
96 publications
7.2K citations
Université Paris Cité
Paris, France
37 h-index
139 publications
8.4K citations
KU Leuven
Leuven, Belgium
37 h-index
132 publications
7K citations
Institute of Astronomy
Moscow, Russia
36 h-index
105 publications
7.6K citations

Observatoire de Paris
Paris, France
35 h-index
117 publications
7.7K citations
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ApJ · 795 publications · 72.5K citations
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428 publications · 25.9K citations
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326 publications · 20.3K citations
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AJ · 224 publications · 12.3K citations
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