Interstellar Gas Cooling
Interstellar Gas Cooling is a physical process in astrophysics whereby thermal energy is radiated away from low-density gas in the diffuse interstellar medium through atomic and molecular line emissions, thereby reducing the gas temperature and influencing the medium’s thermal balance and dynamical evolution.
255
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2017–2026
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Photoelectric heating of interstellar gas
B. T. Draine · The Astrophysical Journal Supplement Series · 1978 · 1.3K citations
Cooling Flows in Clusters of Galaxies
A. C. Fabian · Annual Review of Astronomy and Astrophysics · 1994 · 1.3K citations
Natural Sciences, Astronomy, Physics +13
Evolution of Buoyant Bubbles in M87
E. Churazov, M. Brüggen, Christian Kaiser et al. · The Astrophysical Journal · 2001 · 719 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
18 h-index
48 publications
4.9K citations
Institute of Astronomy
Moscow, Russia
16 h-index
40 publications
2.3K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
30 publications
2K citations
California Institute of Technology
Pasadena, United States
14 h-index
25 publications
2.2K citations

University of Bologna
Bologna, Italy
12 h-index
19 publications
1.6K citations
University of California, Santa Cruz
Santa Cruz, United States
12 h-index
19 publications
706 citations
Max Planck Institute for Astrophysics
Garching, Germany
10 h-index
19 publications
3.9K citations

Durham University
Durham, United Kingdom
9 h-index
21 publications
1.2K citations
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ApJ · 113 publications · 9.7K citations
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