Open Cluster Initial Mass Function
The Open Cluster Initial Mass Function is a statistical representation of the distribution of stellar masses at the time of formation within an open cluster, distinguishing itself from other forms of mass functions by its specific application to gravitationally bound, young stellar populations in galactic disk environments.
36
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1.8K
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68
Authors
59
Institutions
Publications per year
2017–2026
2
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A complete N-body model of the old open cluster M67
Jarrod R. Hurley, O. R. Pols, S. J. Aarseth et al. · 2005 · 149 citations · Full text
Natural Sciences, Astronomy, Physics +17
The White Dwarf Deficit in Open Clusters: Dynamical Processes
The Astrophysical Journal · 2003 · 73 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Main Astronomical Observatory
Kyiv, Ukraine
6 h-index
6 publications
514 citations
Heidelberg University
Heidelberg, Germany
5 h-index
15 publications
867 citations
University of Cambridge
Cambridge, United Kingdom
4 h-index
4 publications
151 citations
Osservatorio Astronomico di Padova
Padua, Italy
4 h-index
6 publications
85 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
4 h-index
11 publications
703 citations
National Astronomical Observatories
Beijing, China
3 h-index
4 publications
200 citations
University of California, Santa Cruz
Santa Cruz, United States
3 h-index
5 publications
235 citations
Institute of Astronomy
Moscow, Russia
3 h-index
6 publications
858 citations
1–8 of 59
11 publications · 667 citations
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8 publications · 403 citations
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ApJ · 4 publications · 172 citations
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AJ · 4 publications · 254 citations
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Repository · 2 publications · 59 citations
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