H I Self-absorption
H I Self-Absorption is a radiative transfer phenomenon in radio astronomy whereby cold atomic hydrogen gas absorbs background 21 cm emission from warmer H I regions, distinguished by its role in revealing the presence and properties of low-temperature, neutral hydrogen clouds in the interstellar medium.
101
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4.7K
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346
Authors
171
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2017–2026
12
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Hisa
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101
KINEMATIC DISTANCES TO MOLECULAR CLOUDS IDENTIFIED IN THE GALACTIC RING SURVEY
Julia Román-Duval, James M. Jackson, M. H. Heyer et al. · The Astrophysical Journal · 2009 · 246 citations · Full text
Natural Sciences, Astronomy, Physics +14
RESOLUTION OF THE DISTANCE AMBIGUITY FOR GALACTIC H II REGIONS
L. D. Anderson, T. M. Bania · The Astrophysical Journal · 2008 · 189 citations · Full text
Natural Sciences, Astronomy, Physics +14
H<scp>i</scp>Narrow Self‐Absorption in Dark Clouds
Di Li, P. F. Goldsmith · The Astrophysical Journal · 2003 · 160 citations · Full text
Natural Sciences, Astronomy, Physics +10
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171
Jet Propulsion Laboratory
Pasadena, United States
9 h-index
14 publications
468 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
8 h-index
12 publications
1.2K citations

University of Calgary
Calgary, Canada
6 h-index
10 publications
604 citations

Cornell University
Ithaca, United States
5 h-index
9 publications
717 citations
National Radio Astronomy Observatory
Charlottesville, United States
5 h-index
7 publications
202 citations
Australia Telescope National Facility
Sydney, Australia
5 h-index
7 publications
434 citations

University of Cologne
Cologne, Germany
5 h-index
21 publications
794 citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
5 h-index
7 publications
434 citations
1–8 of 171
ApJ · 38 publications · 2.2K citations
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16 publications · 565 citations
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6 publications · 194 citations
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AJ · 4 publications · 235 citations
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2 publications · 91 citations
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