Salpeter Initial Mass Function
The Salpeter Initial Mass Function is a power-law model of the initial mass distribution of stellar populations, distinguished by its specific exponent of −2.35, proposed by Edwin E. Salpeter in 1955 to describe the relative number of stars formed per unit mass interval.
285
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26.9K
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678
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365
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Publications per year
2017–2026
50
Variants
Salpeter Imf
Parents
285
Stellar Mass‐to‐Light Ratios and the Tully‐Fisher Relation
The Astrophysical Journal · 2001 · 1.8K citations · Full text
Natural Sciences, Astronomy, Physics +16
The rate of star formation in normal disk galaxies
Jr. Kennicutt R. C. · The Astrophysical Journal · 1983 · 1K citations
Natural Sciences, Astronomy, Physics +15
Galacti chemical evolution: Hygrogen through zinc
The Astrophysical Journal Supplement Series · 1995 · 894 citations · Full text
Natural Sciences, Astronomy, Physics +17
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365

Centre National de la Recherche Scientifique
Paris, France
21 h-index
44 publications
4K citations

Space Telescope Science Institute
Baltimore, United States
17 h-index
40 publications
3.4K citations
University of California, Santa Cruz
Santa Cruz, United States
16 h-index
26 publications
2.8K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
16 h-index
28 publications
1.4K citations
University of Oxford
Oxford, United Kingdom
14 h-index
31 publications
1.9K citations
European Southern Observatory
Garching bei München, Germany
14 h-index
22 publications
1.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
14 h-index
14 publications
3.1K citations
University of Arizona
Tucson, United States
14 h-index
25 publications
2.6K citations
1–8 of 365
ApJ · 74 publications · 9.2K citations
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93 publications · 7.3K citations
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15 publications · 717 citations
15
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AJ · 16 publications · 1.3K citations
14
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10 publications · 531 citations
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