Interstellar Dust Opacity
Interstellar Dust Opacity is a physical quantity that characterizes the attenuation of electromagnetic radiation due to scattering and absorption by interstellar dust grains, distinguished from other opacity sources by its wavelength-dependent interaction with starlight in the diffuse interstellar medium.
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14.2K
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907
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393
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<i>Planck</i>2013 results. XI. All-sky model of thermal dust emission
A. Abergel, P. A. R. Ade, N. Aghanim et al. · Astronomy and Astrophysics · 2014 · 826 citations · Full text
Natural Sciences, Astronomy, Physics +17
On the Submillimeter Opacity of Protoplanetary Disks
B. T. Draine · The Astrophysical Journal · 2006 · 495 citations · Full text
Natural Sciences, Astronomy, Physics +13
Infrared cirrus - New components of the extended infrared emission
F. J. Low, E. T. Young, D. A. Beintema et al. · The Astrophysical Journal · 1984 · 458 citations
Natural Sciences, Astronomy, Physics +17
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Centre National de la Recherche Scientifique
Paris, France
18 h-index
164 publications
68K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
17 h-index
22 publications
3.2K citations
California Institute of Technology
Pasadena, United States
16 h-index
71 publications
25.2K citations

University of Toronto
Toronto, Canada
13 h-index
29 publications
7.1K citations
National Radio Astronomy Observatory
Charlottesville, United States
12 h-index
15 publications
1.5K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
12 h-index
22 publications
1.6K citations
European Southern Observatory
Garching bei München, Germany
12 h-index
13 publications
828 citations
Jet Propulsion Laboratory
Pasadena, United States
12 h-index
29 publications
14.7K citations
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ApJ · 70 publications · 6.2K citations
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22 publications · 1.3K citations
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21 publications · 2.6K citations
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5 publications · 490 citations
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