Nebular Reddening
Nebular Reddening is a systematic observational phenomenon in astrophysics whereby interstellar dust associated with nebular regions preferentially scatters shorter wavelengths of light, leading to an apparent reddening of background starlight distinct from intrinsic stellar spectra or other reddening mechanisms.
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Infrared Observations of Nebular Emission Lines from Galaxies at<i>z</i>≃ 3
Max Pettini, M. Kellogg, Charles C. Steidel et al. · The Astrophysical Journal · 1998 · 341 citations · Full text
Natural Sciences, Astronomy, Physics +16
R. Racine · The Astronomical Journal · 1968 · 199 citations
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Space Telescope Science Institute
Baltimore, United States
6 h-index
16 publications
862 citations
California Institute of Technology
Pasadena, United States
6 h-index
11 publications
1.5K citations
Carnegie Observatories
Pasadena, United States
6 h-index
11 publications
657 citations
University College London
London, United Kingdom
4 h-index
12 publications
721 citations
University of Chile
Santiago, Chile
4 h-index
6 publications
135 citations

University of Hawaii System
Honolulu, United States
4 h-index
5 publications
248 citations
Goddard Space Flight Center
Greenbelt, United States
4 h-index
5 publications
169 citations
University of Maryland, College Park
College Park, United States
4 h-index
4 publications
115 citations
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ApJ · 39 publications · 1.7K citations
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7 publications · 229 citations
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AJ · 3 publications · 390 citations
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