Galactic Mass Distribution
Galactic Mass Distribution is a theoretical construct in astrophysics that specifies the spatial arrangement of stellar, gaseous, dark matter, and total mass components within a galaxy as a function of radius, enabling the modeling of gravitational potentials and rotational dynamics.
779
Publications
71.7K
Citations
1.9K
Authors
602
Institutions
Publications per year
2017–2026
136
Parents
779
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 779
1.9K
13
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11
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11
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Center for Astrophysics Harvard & Smithsonian, United States
11 publications · 2.4K citations
11
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9
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1–5 of 1.9K
602

Centre National de la Recherche Scientifique
Paris, France
34 h-index
115 publications
12.7K citations
Max Planck Institute for Astrophysics
Garching, Germany
25 h-index
56 publications
5.3K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
54 publications
10.6K citations
University of Cambridge
Cambridge, United Kingdom
22 h-index
39 publications
5.3K citations

Durham University
Durham, United Kingdom
22 h-index
84 publications
14.6K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
21 h-index
41 publications
4.2K citations
California Institute of Technology
Pasadena, United States
20 h-index
53 publications
6.1K citations

Chinese Academy of Sciences
Beijing, China
20 h-index
81 publications
4.9K citations
1–8 of 602
ApJ · 269 publications · 28.1K citations
88
h-index
169 publications · 20.2K citations
64
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AJ · 52 publications · 3.5K citations
34
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48 publications · 3.9K citations
33
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Repository · 14 publications · 600 citations
13
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1–5