Intra-cluster Medium
The "Intra-Cluster Medium" is a hot, diffuse plasma that constitutes the dominant baryonic component of galaxy clusters, distinguished by its thermal emission in the X-ray band due to bremsstrahlung radiation from highly ionized ions in hydrostatic equilibrium within the cluster’s gravitational potential.
789
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604
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2017–2026
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789
The Astrophysical Journal · 1999 · 1K citations · Full text
Natural Sciences, Astronomy, Physics +15
Annual Review of Astronomy and Astrophysics · 2012 · 840 citations · Full text
Natural Sciences, Astronomy, Physics +16
Annual Review of Astronomy and Astrophysics · 2002 · 702 citations · Full text
Natural Sciences, Astronomy, Physics +15
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
46 h-index
158 publications
10.7K citations
Max Planck Institute for Astrophysics
Garching, Germany
43 h-index
116 publications
8.2K citations
Istituto di Radioastronomia di Bologna
Bologna, Italy
37 h-index
213 publications
11.8K citations
Leiden University
Leiden, The Netherlands
34 h-index
184 publications
8.8K citations

Centre National de la Recherche Scientifique
Paris, France
33 h-index
184 publications
9.6K citations

Trieste Astronomical Observatory
Trieste, Italy
31 h-index
103 publications
10.8K citations
Kavli Institute for Particle Astrophysics and Cosmology
Menlo Park, United States
31 h-index
67 publications
6.7K citations
Institute of Astronomy
Moscow, Russia
31 h-index
99 publications
11.9K citations
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ApJ · 199 publications · 21.4K citations
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196 publications · 13.1K citations
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122 publications · 6.8K citations
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Repository · 33 publications · 1.2K citations
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Repository · 21 publications · 1.6K citations
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