Hydrodynamic Stellar Models
Hydrodynamic Stellar Models is a computational framework in astrophysics that simulates the time-dependent behavior of stellar interiors and atmospheres by numerically solving the equations of fluid dynamics, radiation transport, and thermodynamics to model the nonlinear pulsational instabilities and mass motions in variable stars.
651
Publications
46K
Citations
1.2K
Authors
526
Institutions
Publications per year
2017–2026
150
Parents
651
<i>KEPLER</i>PLANETS: A TALE OF EVAPORATION
The Astrophysical Journal · 2013 · 771 citations · Full text
Natural Sciences, Astronomy, Physics +15
1–5 of 651
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Centre National de la Recherche Scientifique
Paris, France
29 h-index
153 publications
7.1K citations
Max Planck Institute for Astrophysics
Garching, Germany
25 h-index
77 publications
6.7K citations
Université Paris Cité
Paris, France
17 h-index
47 publications
1.9K citations
Heidelberg University
Heidelberg, Germany
17 h-index
30 publications
1.5K citations

Aarhus University
Aarhus, Denmark
15 h-index
35 publications
1.4K citations
Los Alamos National Laboratory
Los Alamos, United States
14 h-index
25 publications
1.5K citations
The University of Tokyo
Tokyo, Japan
14 h-index
21 publications
666 citations
Institute of Astronomy
Moscow, Russia
14 h-index
32 publications
15K citations
1–8 of 526
ApJ · 191 publications · 14.7K citations
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97 publications · 12.1K citations
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81 publications · 4.5K citations
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26 publications · 814 citations
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Repository · 21 publications · 939 citations
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