Stellar Opacities
Stellar Opacities is a theoretical construct in astrophysics that quantifies the resistance of stellar material to radiative energy transfer, distinguished by its dependence on temperature, density, and chemical composition in modeling the internal structure and evolution of stars.
372
Publications
42.5K
Citations
731
Authors
319
Institutions
Publications per year
2017–2026
40
Parents
372
Carlos A. Iglesias, F. J. Rogers · The Astrophysical Journal · 1996 · 3K citations
Natural Sciences, Astronomy, Physics +14
1–5 of 372
731
Lawrence Livermore National Laboratory, United States
18 publications · 5.7K citations
18
h-index
15
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11
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11
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9
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1–5 of 731
319

Centre National de la Recherche Scientifique
Paris, France
18 h-index
47 publications
3.9K citations
Los Alamos National Laboratory
Los Alamos, United States
14 h-index
72 publications
5.4K citations
University College London
London, United Kingdom
13 h-index
25 publications
2.4K citations

Lawrence Livermore National Laboratory
Livermore, United States
12 h-index
50 publications
6.8K citations

École Normale Supérieure de Lyon
Lyon, France
11 h-index
17 publications
1.2K citations
Yale University
New Haven, United States
11 h-index
13 publications
2.2K citations
Osservatorio Astronomico di Padova
Padua, Italy
11 h-index
22 publications
28.2K citations
Goddard Space Flight Center
Greenbelt, United States
11 h-index
12 publications
895 citations
1–8 of 319
ApJ · 128 publications · 14.4K citations
57
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48 publications · 8.8K citations
35
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38 publications · 3.2K citations
29
h-index
18 publications · 4.3K citations
18
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Repository · 7 publications · 502 citations
7
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1–5