Lognormal Initial Mass Function
The Lognormal Initial Mass Function is a statistical model of stellar initial mass distribution wherein the mass spectrum is described by a lognormal probability density function, distinguished from other forms of the Initial Mass Function by its mathematical characterization of low- to intermediate-mass star formation prevalence.
29
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16.4K
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85
Authors
77
Institutions
Publications per year
2017–2026
3
Variants
Lognormal Imf
Parents
29
Galactic Stellar and Substellar Initial Mass Function
2003 · 4.2K citations
Natural Sciences, Astronomy, Physics +13
Holger Baumgardt, M. Hilker, A. Sollima et al. · Monthly Notices of the Royal Astronomical Society · 2018 · 437 citations · Full text
Natural Sciences, Astronomy, Physics +16
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Centre National de la Recherche Scientifique
Paris, France
4 h-index
9 publications
10.3K citations

École Normale Supérieure de Lyon
Lyon, France
3 h-index
3 publications
9.6K citations
University of Cambridge
Cambridge, United Kingdom
3 h-index
6 publications
179 citations
European Southern Observatory
Garching bei München, Germany
2 h-index
2 publications
468 citations

Space Telescope Science Institute
Baltimore, United States
2 h-index
2 publications
572 citations
Université Claude Bernard Lyon 1
Villeurbanne, France
2 h-index
2 publications
9.6K citations
University of Washington
Seattle, United States
2 h-index
3 publications
182 citations

Université Grenoble Alpes
Saint-Martin-d'Hères, France
2 h-index
3 publications
89 citations
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11 publications · 1.4K citations
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ApJ · 6 publications · 995 citations
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PASP · 2 publications · 9K citations
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1 publications · 393 citations
1
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1 publications · 166 citations
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