Cool Gas Clouds
Cool Gas Clouds is a construct in astrophysics referring to discrete, gravitationally unbound reservoirs of ionized or neutral interstellar medium observed within the circumgalactic medium, distinguished by their relatively low temperatures (typically 10^4 K or below) and high column densities of metal ions, which facilitate the study of gas accretion, feedback, and phase structure in galaxy halos.
276
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18.6K
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811
Authors
328
Institutions
Publications per year
2017–2026
65
Parents
276
Molecular Depletion and Thermal Balance in Dark Cloud Cores
P. F. Goldsmith · The Astrophysical Journal · 2001 · 483 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 276
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
15 h-index
76 publications
9K citations
Institute of Astronomy
Moscow, Russia
15 h-index
35 publications
2.6K citations
University of California, Santa Cruz
Santa Cruz, United States
15 h-index
25 publications
2.3K citations
University of California, Santa Barbara
Santa Barbara, United States
13 h-index
19 publications
2.9K citations
Princeton University
Princeton, United States
13 h-index
17 publications
2K citations

Space Telescope Science Institute
Baltimore, United States
13 h-index
20 publications
1.1K citations
Goddard Space Flight Center
Greenbelt, United States
12 h-index
19 publications
1.5K citations

University of Massachusetts Amherst
Amherst Center, United States
12 h-index
23 publications
1.6K citations
1–8 of 328
ApJ · 119 publications · 8.6K citations
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70 publications · 5.5K citations
35
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9 publications · 579 citations
9
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7 publications · 563 citations
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AJ · 6 publications · 277 citations
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