Foreground Reddening
Foreground Reddening is a type of interstellar extinction process in which ultraviolet radiation from distant astronomical sources is preferentially absorbed and scattered by intervening dust and gas located between the observer and the source, leading to an observed reddening of the source's spectrum.
97
Publications
4.7K
Citations
465
Authors
258
Institutions
Publications per year
2017–2026
11
Parents
97
Solar wind as the origin of rapid reddening of asteroid surfaces
Pierre Vernazza, Richard P. Binzel, A. Rossi et al. · Nature · 2009 · 216 citations
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258
European Southern Observatory
Garching bei München, Germany
8 h-index
11 publications
559 citations
University of Cambridge
Cambridge, United Kingdom
7 h-index
10 publications
717 citations

Space Telescope Science Institute
Baltimore, United States
7 h-index
15 publications
857 citations
California Institute of Technology
Pasadena, United States
6 h-index
13 publications
954 citations
Osservatorio Astronomico di Padova
Padua, Italy
6 h-index
13 publications
948 citations
University of California, Berkeley
Berkeley, United States
6 h-index
7 publications
526 citations
Cerro Tololo Inter-American Observatory
La Serena, Chile
5 h-index
9 publications
576 citations

Observatoire de Paris
Paris, France
5 h-index
9 publications
820 citations
1–8 of 258
ApJ · 28 publications · 1.5K citations
20
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AJ · 14 publications · 560 citations
14
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12 publications · 333 citations
12
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12 publications · 614 citations
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PASP · 5 publications · 133 citations
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