Galaxy Disks
Galaxy Disks is a structural component of spiral and lenticular galaxies characterized by a flattened, rotating distribution of stars, gas, and dust that distinguishes it from the more spheroidal components such as bulges and halos.
1.4K
Publications
129K
Citations
2.8K
Authors
748
Institutions
Publications per year
2017–2026
165
Variants
Galactic Disks
Parents
1.4K
Detailed Structural Decomposition of Galaxy Images
Chien Y. Peng, Luis C. Ho, Chris Impey et al. · The Astronomical Journal · 2002 · 2.8K citations · Full text
Natural Sciences, Astronomy, Physics +12
On the Disks of Spiral and so Galaxies
K. C. Freeman · The Astrophysical Journal · 1970 · 2.1K citations
Natural Sciences, Astronomy, Physics +15
1–5 of 1.4K
2.8K
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748
California Institute of Technology
Pasadena, United States
50 h-index
148 publications
17K citations

Space Telescope Science Institute
Baltimore, United States
46 h-index
177 publications
13.5K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
45 h-index
158 publications
11.6K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
43 h-index
148 publications
22.4K citations

Centre National de la Recherche Scientifique
Paris, France
42 h-index
190 publications
14.3K citations
University of Arizona
Tucson, United States
41 h-index
105 publications
17.1K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
40 h-index
189 publications
35.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
37 h-index
99 publications
7.7K citations
1–8 of 748
ApJ · 588 publications · 61.1K citations
123
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AJ · 168 publications · 16.4K citations
66
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103 publications · 11.1K citations
53
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129 publications · 8K citations
49
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42 publications · 4.8K citations
35
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