Disk Decomposition
Disk Decomposition is a methodological approach in astrophysics that separates the observed rotation curve of a galaxy into distinct kinematic contributions from its structural components, primarily the stellar disk, gas disk, and dark matter halo, to determine their individual mass distributions.
92
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9.6K
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383
Authors
220
Institutions
Publications per year
2017–2026
18
Parents
92
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
H. Salo, E. Laurikainen, Jarkko Laine et al. · The Astrophysical Journal Supplement Series · 2015 · 305 citations · Full text
Natural Sciences, Astronomy, Physics +12
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Centre National de la Recherche Scientifique
Paris, France
11 h-index
47 publications
3.2K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
10 h-index
27 publications
2.4K citations

Space Telescope Science Institute
Baltimore, United States
9 h-index
12 publications
1.1K citations
European Southern Observatory
Santiago, Chile
8 h-index
16 publications
1.9K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
8 h-index
14 publications
4K citations
University of California, Santa Cruz
Santa Cruz, United States
7 h-index
24 publications
1.5K citations
European Southern Observatory
Garching bei München, Germany
7 h-index
12 publications
948 citations
Max Planck Society
Munich, Germany
7 h-index
12 publications
3.5K citations
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31 publications · 2K citations
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ApJ · 16 publications · 1.6K citations
15
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16 publications · 617 citations
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AJ · 10 publications · 3.3K citations
10
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3 publications · 1K citations
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