Open Cluster Dissolution
Open Cluster Dissolution is a theoretical construct in astrophysics that denotes the gradual dispersal of stars from an open cluster due to internal dynamical processes, external tidal forces, and stellar evolution, leading to the loss of gravitational coherence and eventual integration of member stars into the galactic field population.
29
Publications
1.4K
Citations
54
Authors
41
Institutions
Publications per year
2017–2026
7
Variants
Open Cluster Dispersal
Parents
29
The age of the oldest Open Clusters
Astronomy and Astrophysics · 2004 · 199 citations · Full text
Natural Sciences, Astronomy, Physics +17
Evidence for Primordial Mass Segregation in Globular Clusters
The Astrophysical Journal · 2008 · 115 citations · Full text
Natural Sciences, Astronomy, Physics +17
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41
Universidade Federal do Rio Grande do Sul
Porto Alegre, Brazil
5 h-index
18 publications
614 citations
University of Bonn
Bonn, Germany
5 h-index
8 publications
636 citations
Osservatorio Astronomico di Padova
Padua, Italy
4 h-index
5 publications
85 citations
Suffolk University Madrid
Madrid, Spain
4 h-index
8 publications
210 citations

University of Padua
Padua, Italy
4 h-index
5 publications
85 citations

Consejo Nacional de Investigaciones Científicas y Técnicas
Buenos Aires, Argentina
3 h-index
4 publications
62 citations
Federal Center for Technological Education of Minas Gerais
Belo Horizonte, Brazil
3 h-index
3 publications
53 citations

European Space Research and Technology Centre
Noordwijk-Binnen, The Netherlands
3 h-index
3 publications
150 citations
1–8 of 41
11 publications · 413 citations
10
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3 publications · 89 citations
3
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Repository · 3 publications · 40 citations
3
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AJ · 2 publications · 133 citations
2
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ApJ · 2 publications · 173 citations
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