Non-keplerian Orbits
Non-Keplerian Orbits is a theoretical construct in orbital dynamics that denotes a satellite orbit trajectory that deviates from the classical two-body gravitational solution due to continuous propulsion or persistent perturbative forces, thereby maintaining a non-Keplerian path unlike natural or impulsive maneuver-based orbits.
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2017–2026
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Thick accretion disks with super-Eddington luminosities
M. A. Abramowicz, M. Calvani, L. Nobili · The Astrophysical Journal · 1980 · 195 citations
Natural Sciences, Astronomy, Physics +16
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147

Centre National de la Recherche Scientifique
Paris, France
7 h-index
10 publications
322 citations

University of Glasgow
Glasgow, United Kingdom
6 h-index
7 publications
310 citations

University of Strathclyde
Glasgow, United Kingdom
6 h-index
15 publications
855 citations
Max Planck Society
Munich, Germany
5 h-index
5 publications
220 citations

University of Göttingen
Göttingen, Germany
5 h-index
19 publications
989 citations

University of Pisa
Pisa, Italy
4 h-index
10 publications
366 citations
University of Chile
Santiago, Chile
4 h-index
13 publications
1.2K citations
University of Geneva
Geneva, Switzerland
4 h-index
7 publications
236 citations
1–8 of 147
12 publications · 454 citations
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11 publications · 489 citations
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11 publications · 454 citations
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ApJ · 7 publications · 454 citations
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Repository · 4 publications · 60 citations
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