Gas Cooling Processes
Gas Cooling Processes is a physical mechanism within the broader class of energy dissipation phenomena in interstellar media, distinguished by the emission of infrared and submillimeter radiation from atoms and molecules in photodissociated gas that results from far-ultraviolet radiation-induced excitation and subsequent radiative decay, thereby reducing the thermal energy of the region.
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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
Cooling of gases by laser radiation
T. W. Hänsch, A. L. Schawlow · Optics Communications · 1975 · 1K citations · Full text
What Shapes the Luminosity Function of Galaxies?
Andrew Benson, R. G. Bower, Carlos S. Frenk et al. · The Astrophysical Journal · 2003 · 888 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
26 h-index
69 publications
6.8K citations

Centre National de la Recherche Scientifique
Paris, France
25 h-index
61 publications
4K citations

Durham University
Durham, United Kingdom
24 h-index
90 publications
13K citations
Max Planck Institute for Astrophysics
Garching, Germany
23 h-index
45 publications
8.2K citations
California Institute of Technology
Pasadena, United States
23 h-index
44 publications
5.8K citations
Leiden University
Leiden, The Netherlands
22 h-index
50 publications
5.1K citations
Institute of Astronomy
Moscow, Russia
19 h-index
49 publications
2.8K citations
University of Cambridge
Cambridge, United Kingdom
17 h-index
33 publications
2.3K citations
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ApJ · 125 publications · 13.5K citations
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