Disk Precession is a dynamical phenomenon in accretion disk physics wherein the orbital plane of the disk undergoes a slow, coherent rotation about the angular momentum axis of the central gravitating body, distinguishing it from other forms of precession by its collective, large-scale articulation of disk material due to relativistic or gravitational perturbations.
71
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240
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150
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2017–2026
17
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71
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Authors
240
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5
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4
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3
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2
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2
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150
University of Cambridge
Cambridge, United Kingdom
6 h-index
14 publications
1.7K citations
Cornell University
Ithaca, United States
5 h-index
9 publications
538 citations
Columbia University
New York, United States
4 h-index
5 publications
506 citations
Canadian Institute for Theoretical Astrophysics
Toronto, Canada
4 h-index
4 publications
100 citations
Instituto Argentino de Radioastronomía
Buenos Aires, Argentina
4 h-index
3 publications
80 citations
Goddard Space Flight Center
Greenbelt, United States
4 h-index
8 publications
432 citations
Massachusetts Institute of Technology
Cambridge, United States
3 h-index
3 publications
228 citations
Florida Institute of Technology
Melbourne, United States
3 h-index
4 publications
164 citations
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- The Astrophysical Journal
ApJ · 25 publications · 1.6K citations
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- Monthly Notices of the Royal Astronomical Society
12 publications · 1K citations
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- Astronomy and Astrophysics
6 publications · 134 citations
6
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- CERN Document Server (European Organization for Nuclear Research)
Repository · 5 publications · 253 citations
5
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- Publications of the Astronomical Society of the Pacific
PASP · 3 publications · 441 citations
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