Bulge Stellar Orbits
Bulge Stellar Orbits is a theoretical construct in astrophysics that describes the characteristic trajectories of stars within the galactic bulge, distinguished by their predominantly radial and anisotropic motions influenced by the bulge’s non-axisymmetric gravitational potential.
41
Publications
2.2K
Citations
117
Authors
86
Institutions
Publications per year
2017–2026
11
Parents
41
Imprints of fast-rotating massive stars in the Galactic Bulge
C. Chiappini, U. Frischknecht, G. Meynet et al. · Nature · 2011 · 156 citations
Natural Sciences, Astronomy, Physics +13
Transiting extrasolar planetary candidates in the Galactic bulge
K. C. Sahu, Stefano Casertano, Howard E. Bond et al. · Nature · 2006 · 148 citations · Full text
Natural Sciences, Astronomy, Physics +11
1–5 of 41
117
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Max Planck Institute for Extraterrestrial Physics, Germany
3 publications · 232 citations
3
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3
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3
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3
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1–5 of 117
86

Shanghai Astronomical Observatory
Shanghai, China
6 h-index
12 publications
410 citations
University of California, Los Angeles
Los Angeles, United States
6 h-index
6 publications
289 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
5 h-index
6 publications
299 citations
Universidade de São Paulo
São Paulo, Brazil
4 h-index
7 publications
400 citations
Columbia University
New York, United States
4 h-index
10 publications
603 citations
Universidade Cidade de São Paulo
São Paulo, Brazil
4 h-index
7 publications
400 citations
Heidelberg University
Heidelberg, Germany
3 h-index
5 publications
129 citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
3 h-index
12 publications
1.3K citations
1–8 of 86
11 publications · 459 citations
11
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ApJ · 9 publications · 583 citations
9
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5 publications · 258 citations
5
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AJ · 4 publications · 217 citations
4
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2 publications · 304 citations
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