Initial Mass Function In Open Clusters
Initial Mass Function in Open Clusters is a statistical model that describes the distribution of stellar masses at birth within open star clusters, distinguishing itself from broader initial mass functions by specifically characterizing the mass distribution in the low-density, galactic disk environments typical of open clusters.
27
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1.6K
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68
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62
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2017–2026
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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
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National Astronomical Observatories
Beijing, China
3 h-index
4 publications
150 citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
3 publications
138 citations

Chinese Academy of Sciences
Beijing, China
3 h-index
4 publications
150 citations
Institute of Astronomy
Moscow, Russia
3 h-index
7 publications
830 citations

UNSW Sydney
Sydney, Australia
2 h-index
2 publications
45 citations
Utrecht University
Utrecht, The Netherlands
2 h-index
2 publications
391 citations

Leibniz Institute for Astrophysics Potsdam
Potsdam, Germany
2 h-index
7 publications
290 citations
Main Astronomical Observatory
Kyiv, Ukraine
2 h-index
2 publications
78 citations
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8 publications · 330 citations
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ApJ · 5 publications · 371 citations
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AJ · 5 publications · 325 citations
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4 publications · 320 citations
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2 publications · 28 citations
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