Bulge Density Profiles
Bulge Density Profiles is a theoretical astrophysical model that characterizes the spatial distribution of stellar mass within the central region of a galaxy by specifying how density varies with distance from the galactic center, distinguishing it from disk or halo density models through its focus on the spheroidal bulge component.
62
Publications
6.1K
Citations
132
Authors
109
Institutions
Publications per year
2017–2026
12
Parents
62
Analytical models for galactic nuclei
Hongsheng Zhao · Monthly Notices of the Royal Astronomical Society · 1996 · 654 citations · Full text
Natural Sciences, Astronomy, Physics +15
Systematics of bulge-to-disk ratios
F. Simien · The Astrophysical Journal · 1986 · 376 citations
Natural Sciences, Astronomy, Physics +15
1–5 of 62
132
Max Planck Institute for Extraterrestrial Physics, Germany
7 publications · 1.1K citations
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4
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4
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3
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3
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1–5 of 132
109

Centre National de la Recherche Scientifique
Paris, France
7 h-index
10 publications
554 citations
European Southern Observatory
Garching bei München, Germany
6 h-index
14 publications
854 citations
Princeton University
Princeton, United States
6 h-index
7 publications
498 citations
Pontificia Universidad Católica de Chile
Santiago, Chile
6 h-index
11 publications
1.1K citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
5 h-index
11 publications
610 citations
Carnegie Observatories
Pasadena, United States
5 h-index
6 publications
415 citations
Vatican Observatory
Castel Gandolfo, Italy
5 h-index
5 publications
428 citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
5 h-index
11 publications
1.1K citations
1–8 of 109
21 publications · 3.6K citations
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ApJ · 8 publications · 822 citations
8
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7 publications · 348 citations
7
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Repository · 3 publications · 374 citations
3
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JGR · 3 publications · 49 citations
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1–5