Chabrier Initial Mass Function
The Chabrier Initial Mass Function is a lognormal functional form of the initial mass function introduced by Chabrier that describes the distribution of stellar masses at birth within a population of stars, distinguished from other parameterizations by its probabilistic modeling of star formation processes across both substellar and stellar regimes.
27
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2.1K
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78
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72
Institutions
Publications per year
2017–2026
5
Variants
Chabrier Imf
Parents
27
THE INITIAL MASS FUNCTION OF EARLY-TYPE GALAXIES
Tommaso Treu, Matthew W. Auger, L. V. E. Koopmans et al. · The Astrophysical Journal · 2010 · 411 citations · Full text
Natural Sciences, Astronomy, Physics +14
Towards initial mass functions for asteroids and Kuiper Belt Objects
Jeffrey N. Cuzzi, R. C. Hogan, W. F. Bottke · Icarus · 2010 · 166 citations · Full text
Natural Sciences, Astronomy, Physics +10
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Centre National de la Recherche Scientifique
Paris, France
5 h-index
7 publications
897 citations

University of Massachusetts Amherst
Amherst Center, United States
4 h-index
7 publications
410 citations
University College London
London, United Kingdom
3 h-index
3 publications
110 citations
Institut d'Astrophysique de Paris
Paris, France
3 h-index
3 publications
747 citations
National Astronomical Observatories
Beijing, China
3 h-index
4 publications
106 citations

University of Exeter
Exeter, United Kingdom
3 h-index
3 publications
177 citations
University of California, Riverside
Riverside, United States
2 h-index
3 publications
51 citations
Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères
Paris, France
2 h-index
2 publications
44 citations
1–8 of 72
13 publications · 873 citations
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ApJ · 5 publications · 859 citations
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AJ · 1 publications · 21 citations
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1 publications · 48 citations
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1 publications · 17 citations
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