Interstellar Cooling
Interstellar Cooling is a physical process in astrophysics wherein thermal energy is radiated away from the interstellar medium through electromagnetic emissions, primarily via atomic and molecular line radiation, thereby reducing the gas temperature and regulating star formation and cloud dynamics.
62
Publications
7.6K
Citations
129
Authors
59
Institutions
Publications per year
2017–2026
4
62
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
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129
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Joint Institute for Laboratory Astrophysics, United States
2 publications · 477 citations
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University of Bologna
Bologna, Italy
4 h-index
4 publications
90 citations
Massachusetts Institute of Technology
Cambridge, United States
4 h-index
6 publications
524 citations
Osservatorio astronomico di Bologna
Bologna, Italy
4 h-index
4 publications
90 citations
University of California, Santa Cruz
Santa Cruz, United States
4 h-index
7 publications
150 citations
Max Planck Society
Munich, Germany
2 h-index
2 publications
420 citations
Institute of Applied Physics
Nizhny Novgorod, Russia
2 h-index
2 publications
69 citations
Cardiff University
Cardiff, United Kingdom
2 h-index
4 publications
64 citations
National Radio Astronomy Observatory
Charlottesville, United States
2 h-index
2 publications
123 citations
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ApJ · 37 publications · 3.6K citations
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5 publications · 162 citations
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2 publications · 32 citations
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2 publications · 1.3K citations
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1 publications · 14 citations
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