Star Cluster Extinction
Star Cluster Extinction is a systematic observational bias in astrophysics that refers to the dimming and reddening of star cluster light caused by the absorption and scattering of photons by intervening interstellar dust and gas along the line of sight.
178
Publications
8.1K
Citations
549
Authors
279
Institutions
Publications per year
2017–2026
18
Parents
178
Surface brightness profile of the Milky Way’s nuclear star cluster
R. Schödel, A. Feldmeier, D. Kunneriath et al. · Astronomy and Astrophysics · 2014 · 205 citations · Full text
Natural Sciences, Astronomy, Physics +15
The star cluster population of M 51
N. Bastian, Mark Gieles, H. J. G. L. M. Lamers et al. · Astronomy and Astrophysics · 2005 · 199 citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 178
549
9
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9
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8
h-index
Aryabhatta Research Institute of Observational Sciences, India
6 publications · 121 citations
6
h-index
5
h-index
1–5 of 549
279

Space Telescope Science Institute
Baltimore, United States
20 h-index
41 publications
1.8K citations
European Southern Observatory
Garching bei München, Germany
11 h-index
18 publications
1.5K citations
University of Wisconsin–Madison
Madison, United States
10 h-index
14 publications
653 citations
University of Arizona
Tucson, United States
9 h-index
21 publications
957 citations

Chinese Academy of Sciences
Beijing, China
9 h-index
17 publications
456 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
25 publications
1.4K citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
13 publications
1K citations
European Southern Observatory
Santiago, Chile
8 h-index
8 publications
217 citations
1–8 of 279
41 publications · 1.9K citations
26
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AJ · 36 publications · 1.6K citations
24
h-index
ApJ · 33 publications · 1.4K citations
21
h-index
31 publications · 1.9K citations
21
h-index
Repository · 8 publications · 332 citations
8
h-index
1–5