Cuspy Halo Models
Cuspy Halo Models is a theoretical astrophysical framework characterized by a predicted density profile of dark matter halos that increases sharply toward the galactic center, thereby producing a "cusp" in contrast to observed rotation curves that suggest a more uniform central density.
153
Publications
13.3K
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367
Authors
254
Institutions
Publications per year
2017–2026
31
Parents
153
The unexpected diversity of dwarf galaxy rotation curves
Kyle A. Oman, Julio F. Navarro, Azadeh Fattahi et al. · Monthly Notices of the Royal Astronomical Society · 2015 · 471 citations · Full text
Natural Sciences, Astronomy, Physics +14
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University of Cambridge
Cambridge, United Kingdom
12 h-index
26 publications
4.2K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
39 publications
1.3K citations
University of Zurich
Zurich, Switzerland
9 h-index
18 publications
2.3K citations
University of Oxford
Oxford, United Kingdom
8 h-index
11 publications
1.4K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
8 h-index
11 publications
882 citations
University of Washington
Seattle, United States
7 h-index
14 publications
1.6K citations

Durham University
Durham, United Kingdom
6 h-index
22 publications
5.7K citations

University of Victoria
Victoria, Canada
6 h-index
10 publications
1.7K citations
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54 publications · 5.5K citations
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ApJ · 30 publications · 3.4K citations
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JCAP · 9 publications · 414 citations
9
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8 publications · 641 citations
8
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6 publications · 259 citations
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