Star Cluster Initial Mass Function
The Star Cluster Initial Mass Function is a statistical distribution function that specifies the relative number of star clusters formed per unit initial mass interval, distinguishing it from other mass functions by characterizing the primordial mass distribution of entire clusters rather than individual stars.
165
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22.3K
Citations
310
Authors
217
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2017–2026
20
165
On the variation of the initial mass function
Pavel Kroupa · Monthly Notices of the Royal Astronomical Society · 2001 · 7.5K citations · Full text
Natural Sciences, Astronomy, Physics +16
The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
Pavel Kroupa · Science · 2002 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +17
Star Formation in the Orion Nebula Cluster
F. Palla, Steven W. Stahler · The Astrophysical Journal · 1999 · 570 citations
Natural Sciences, Astronomy, Physics +17
Galactic‐Field Initial Mass Functions of Massive Stars
Pavel Kroupa, C. Weidner · The Astrophysical Journal · 2003 · 524 citations · Full text
Natural Sciences, Astronomy, Physics +16
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217
University of Bonn
Bonn, Germany
22 h-index
42 publications
3.5K citations
University of Cambridge
Cambridge, United Kingdom
11 h-index
21 publications
2.1K citations
Heidelberg University
Heidelberg, Germany
11 h-index
19 publications
1.2K citations
Utrecht University
Utrecht, The Netherlands
11 h-index
32 publications
3.3K citations
University of Arizona
Tucson, United States
10 h-index
20 publications
2K citations
Institute of Astronomy
Moscow, Russia
10 h-index
21 publications
1.3K citations
European Southern Observatory
Santiago, Chile
8 h-index
10 publications
674 citations
University of Michigan
Ann Arbor, United States
8 h-index
15 publications
966 citations
1–8 of 217
57 publications · 11K citations
33
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ApJ · 43 publications · 4.2K citations
31
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22 publications · 1.8K citations
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AJ · 9 publications · 717 citations
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Repository · 6 publications · 207 citations
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