Initial Mass Function In Globular Clusters
The Initial Mass Function in Globular Clusters is a stellar population model that specifies the distribution of stellar masses at the time of formation within globular clusters, distinguishing itself from field star or open cluster initial mass functions by reflecting the unique dynamical and chemical environments of ancient, dense, metal-poor systems.
165
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25K
Citations
306
Authors
212
Institutions
Publications per year
2017–2026
29
Parents
165
Galactic Stellar and Substellar Initial Mass Function
2003 · 4.2K citations
Natural Sciences, Astronomy, Physics +13
1–5 of 165
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Czech Academy of Sciences, Astronomical Institute, Czechia
5 publications · 122 citations
5
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1–5 of 306
212
University of Bonn
Bonn, Germany
14 h-index
25 publications
2.2K citations
European Southern Observatory
Garching bei München, Germany
12 h-index
15 publications
1.1K citations

The University of Queensland
Brisbane, Australia
11 h-index
11 publications
1.1K citations
University of Cambridge
Cambridge, United Kingdom
10 h-index
13 publications
1.6K citations

University of Surrey
Guildford, United Kingdom
8 h-index
13 publications
1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
7 h-index
9 publications
1.7K citations
Osservatorio astronomico di Bologna
Bologna, Italy
7 h-index
10 publications
827 citations

University of Edinburgh
Edinburgh, United Kingdom
7 h-index
10 publications
929 citations
1–8 of 212
59 publications · 5.6K citations
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ApJ · 40 publications · 2.3K citations
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10 publications · 881 citations
9
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7 publications · 274 citations
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5 publications · 325 citations
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