Star Cluster Dissolution is a theoretical construct in astrophysics that denotes the process by which a gravitationally bound star cluster loses its cohesion due to internal dynamics and external tidal forces, resulting in the dispersal of its stellar members into the surrounding galactic environment.
83
Publications
5.3K
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124
Authors
116
Institutions
Publications per year
2017–2026
17
Parents
Publications
83
The dynamical evolution of globular clusters
Alan P. Lightman, Stuart L. Shapiro · Reviews of Modern Physics · 1978 · 165 citations
Natural Sciences, Astronomy, Physics +17
1–5 of 83
Authors
124
- HB
10
h-index
- MG
6
h-index
- HJ
5
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- PK
5
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- PA
4
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1–5 of 124
Institutions
116
University of Bonn
Bonn, Germany
14 h-index
22 publications
1.9K citations
Heidelberg University
Heidelberg, Germany
10 h-index
22 publications
768 citations
Utrecht University
Utrecht, The Netherlands
8 h-index
13 publications
798 citations
Universidade Federal do Rio Grande do Sul
Porto Alegre, Brazil
5 h-index
19 publications
705 citations
Peking University
Beijing, China
5 h-index
6 publications
412 citations
University of Sheffield
Sheffield, United Kingdom
5 h-index
10 publications
757 citations
European Southern Observatory
Santiago, Chile
5 h-index
5 publications
512 citations
Kavli Institute for Theoretical Sciences
Beijing, China
5 h-index
6 publications
412 citations
1–8 of 116
Venues
- Monthly Notices of the Royal Astronomical Society
31 publications · 2.3K citations
22
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- The Astrophysical Journal
ApJ · 15 publications · 1.2K citations
14
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- Astronomy and Astrophysics
13 publications · 524 citations
12
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- Springer Link (Chiba Institute of Technology)
Repository · 3 publications · 115 citations
3
h-index
- The Astronomical Journal
AJ · 2 publications · 54 citations
2
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1–5