Molecular Cloud Extinction
Molecular Cloud Extinction is a specific type of interstellar extinction characterized by the selective absorption and scattering of electromagnetic radiation due to the dense concentration of dust and gas within molecular clouds, distinguishing it from diffuse interstellar medium extinction by its significantly higher opacity and localized spatial distribution.
141
Publications
11.4K
Citations
332
Authors
198
Institutions
Publications per year
2017–2026
10
Parents
141
D. J. Hollenbach, Christopher F. McKee · The Astrophysical Journal · 2010 · 717 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 141
332
Center for Astrophysics Harvard & Smithsonian, United States
18 publications · 1.9K citations
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5
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198
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
21 h-index
38 publications
3.3K citations

University of Milan
Milan, Italy
13 h-index
14 publications
910 citations

Centre National de la Recherche Scientifique
Paris, France
11 h-index
36 publications
1.7K citations
European Southern Observatory
Garching bei München, Germany
11 h-index
12 publications
1.2K citations
University of Vienna
Vienna, Austria
10 h-index
11 publications
530 citations
California Institute of Technology
Pasadena, United States
10 h-index
15 publications
867 citations
University of Florida
Gainesville, United States
9 h-index
12 publications
1.3K citations
Jet Propulsion Laboratory
Pasadena, United States
8 h-index
16 publications
1.9K citations
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ApJ · 60 publications · 6.8K citations
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24 publications · 1.4K citations
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11 publications · 351 citations
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AJ · 9 publications · 730 citations
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Repository · 6 publications · 252 citations
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