Stellar Hydrostatic Equilibrium
Stellar Hydrostatic Equilibrium is a theoretical construct in astrophysics denoting the state in which the inward gravitational force at every point within a star is exactly balanced by the outward pressure gradient force, thereby maintaining the star's stable, spherical structure against collapse or expansion.
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2017–2026
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A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
B. Gustafsson, B. Edvardsson, Åke Nordlund et al. · ArXiv.org · 2008 · 1.3K citations · Full text
Natural Sciences, Astronomy, Physics +16
Hydrostatic Equilibrium of Hypothetical Quark Stars
Naoki Itoh · Progress of Theoretical Physics · 1970 · 825 citations · Full text
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
15 h-index
25 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
26 publications
1.5K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
11 h-index
26 publications
2.1K citations
University of Lisbon
Lisbon, Portugal
9 h-index
16 publications
541 citations
California Institute of Technology
Pasadena, United States
8 h-index
20 publications
1.6K citations
Private University of the North
Trujillo, Peru
8 h-index
8 publications
445 citations
Institute of Astrophysics and Space Sciences
Porto, Portugal
7 h-index
13 publications
363 citations
Instituto Tecnológico de Aeronáutica
São José dos Campos, Brazil
7 h-index
18 publications
1.2K citations
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ApJ · 94 publications · 5K citations
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28 publications · 2K citations
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42 publications · 1.6K citations
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