Epicyclic Approximation
Epicyclic Approximation is a mathematical model in galactic kinematics that describes the motion of stars near a circular orbit in a disk galaxy by approximating their trajectories as small oscillations (epicycles) superposed on the dominant circular motion, thereby simplifying the analysis of stellar orbits in axisymmetric gravitational potentials.
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Non-linear coupling of spiral modes in disc galaxies
J.-F. Sygnet, M. Tagger, E. Athanassoula et al. · Monthly Notices of the Royal Astronomical Society · 1988 · 81 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
5 publications
211 citations
Heidelberg University
Heidelberg, Germany
5 h-index
15 publications
740 citations
Institut d'Astrophysique de Paris
Paris, France
4 h-index
9 publications
282 citations
AlbaNova
Stockholm, Sweden
3 h-index
6 publications
126 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
4 publications
101 citations

Centre National de la Recherche Scientifique
Paris, France
3 h-index
5 publications
133 citations
Consejo Superior de Investigaciones Científicas
Madrid, Spain
2 h-index
2 publications
64 citations
Canadian Institute for Theoretical Astrophysics
Toronto, Canada
2 h-index
2 publications
75 citations
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12 publications · 752 citations
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ApJ · 8 publications · 265 citations
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AJ · 4 publications · 125 citations
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2 publications · 82 citations
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