Halo Decomposition
Halo Decomposition is a computational framework in astrophysics that decomposes the rotation curve of a galaxy into distinct dynamical components—such as stellar, gaseous, and dark matter halo contributions—to isolate and characterize the gravitational influence of the dark matter halo.
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2.8K
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145
Authors
96
Institutions
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2017–2026
8
Parents
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Dark matter in spiral galaxies. I - Galaxies with optical rotation curves
S. Kent · The Astronomical Journal · 1986 · 281 citations
Natural Sciences, Astronomy, Physics +17
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The University of Tokyo
Tokyo, Japan
5 h-index
5 publications
434 citations

Lawrence Berkeley National Laboratory
Berkeley, United States
4 h-index
5 publications
278 citations

Kavli Institute for the Physics and Mathematics of the Universe
Kashiwa, Japan
4 h-index
4 publications
121 citations
University of Washington
Seattle, United States
4 h-index
8 publications
965 citations
University of Utah
Salt Lake City, United States
3 h-index
4 publications
346 citations

Centre National de la Recherche Scientifique
Paris, France
3 h-index
12 publications
575 citations
International Centre for Radio Astronomy Research
Crawley, Australia
3 h-index
6 publications
370 citations

The University of Western Australia
Perth, Australia
3 h-index
6 publications
370 citations
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14 publications · 547 citations
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ApJ · 7 publications · 671 citations
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JCAP · 3 publications · 87 citations
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3 publications · 96 citations
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2 publications · 129 citations
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