Two-Body Relaxation is a dynamical process in stellar systems, specifically within globular clusters, wherein gravitational encounters between pairs of stars gradually alter their trajectories, leading to a redistribution of energy and momentum that drives the system toward thermal equilibrium over time.
187
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13.5K
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351
Authors
216
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Publications per year
2017–2026
36
Publications
187
1–5 of 187
Authors
351
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10
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6
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6
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6
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5
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1–5 of 351
Institutions
216
University of Bonn
Bonn, Germany
11 h-index
19 publications
1.7K citations
University of Edinburgh
Edinburgh, United Kingdom
10 h-index
15 publications
983 citations
European Space Research and Technology Centre
Noordwijk-Binnen, The Netherlands
10 h-index
13 publications
772 citations
Northwestern University
Evanston, United States
7 h-index
13 publications
882 citations
Peking University
Beijing, China
7 h-index
8 publications
262 citations
Space Telescope Science Institute
Baltimore, United States
6 h-index
8 publications
1.1K citations
University of Surrey
Guildford, United Kingdom
6 h-index
12 publications
1.7K citations
Kavli Institute for Theoretical Sciences
Beijing, China
6 h-index
6 publications
160 citations
1–8 of 216
Venues
- Monthly Notices of the Royal Astronomical Society
63 publications · 5.4K citations
38
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- The Astrophysical Journal
ApJ · 48 publications · 4.3K citations
34
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- Publications of the Astronomical Society of Japan
4 publications · 111 citations
4
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- Monthly Notices of the Royal Astronomical Society Letters
4 publications · 186 citations
4
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- Astronomy and Astrophysics
4 publications · 264 citations
4
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