Disk Coronae
Disk Coronae is a theoretical construct in accretion physics denoting a high-temperature, low-density plasma region above and below an accretion disk that thermally and radiatively couples with the disk, distinguishing it from the cooler, denser disk material through its non-thermal emission processes and role in X-ray radiation.
113
Publications
7.3K
Citations
276
Authors
158
Institutions
Publications per year
2017–2026
20
113
X-ray astronomy of stellar coronae
M. G�del · The Astronomy and Astrophysics Review · 2004 · 418 citations · Full text
Natural Sciences, Astronomy, Physics +11
N. E. White, S. S. Holt · The Astrophysical Journal · 1982 · 260 citations
Natural Sciences, Astronomy, Physics +15
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Joint Institute for Laboratory Astrophysics, United States
3 publications · 166 citations
3
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1–5 of 276
158

Kyoto University
Kyoto, Japan
6 h-index
9 publications
424 citations
Nicolaus Copernicus Astronomical Center
Warsaw, Poland
5 h-index
8 publications
281 citations

Lawrence Livermore National Laboratory
Livermore, United States
5 h-index
5 publications
186 citations
The University of Tokyo
Tokyo, Japan
5 h-index
6 publications
215 citations

Centre National de la Recherche Scientifique
Paris, France
5 h-index
8 publications
541 citations
Max Planck Institute for Astrophysics
Garching, Germany
5 h-index
9 publications
480 citations
Princeton University
Princeton, United States
5 h-index
8 publications
557 citations
California Institute of Technology
Pasadena, United States
5 h-index
6 publications
308 citations
1–8 of 158
ApJ · 47 publications · 3.2K citations
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13 publications · 917 citations
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6 publications · 199 citations
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Repository · 5 publications · 547 citations
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3 publications · 273 citations
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