Dust Emissivity
Dust Emissivity is a physical property that quantifies the efficiency with which interstellar dust grains emit electromagnetic radiation per unit mass at a given wavelength, distinguishing it from other emission processes by its dependence on grain composition, size distribution, and temperature.
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2017–2026
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Electric Dipole Radiation from Spinning Dust Grains
The Astrophysical Journal · 1998 · 474 citations · Full text
Natural Sciences, Astronomy, Physics +16
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Centre National de la Recherche Scientifique
Paris, France
41 h-index
527 publications
52.1K citations
California Institute of Technology
Pasadena, United States
36 h-index
120 publications
14.3K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
30 h-index
157 publications
16.2K citations
Astrophysique, Instrumentation et Modélisation
Gif-sur-Yvette, France
28 h-index
143 publications
14.8K citations
Cardiff University
Cardiff, United Kingdom
27 h-index
135 publications
8.8K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
25 h-index
69 publications
6.4K citations
Université Paris Cité
Paris, France
24 h-index
129 publications
15.3K citations
Université Paris-Sud
Orsay, France
22 h-index
126 publications
14.4K citations
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ApJ · 74 publications · 7.4K citations
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58 publications · 4.7K citations
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37 publications · 2.1K citations
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AJ · 8 publications · 178 citations
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5 publications · 257 citations
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