Mass-luminosity Relation
The Mass-Luminosity Relation is an empirical astrophysical law that expresses the quantitative correlation between the mass and luminosity of main-sequence stars, specifying that luminosity scales approximately as a power of the stellar mass.
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713
Institutions
Publications per year
2017–2026
114
Variants
Mass-luminosity Relationship
Parents
790
The Luminosity Function and Stellar Evolution.
E. E. Salpeter · The Astrophysical Journal · 1955 · 8.7K citations
Natural Sciences, Astronomy, Physics +16
A Relationship Between Nuclear Black Hole Mass And Galaxy Velocity Dispersion
2000 · 2.2K citations
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Max Planck Institute for Extraterrestrial Physics, Germany
8 publications · 948 citations
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
34 h-index
85 publications
7.3K citations
California Institute of Technology
Pasadena, United States
30 h-index
59 publications
6.1K citations

Centre National de la Recherche Scientifique
Paris, France
28 h-index
137 publications
7.5K citations
University of California, Berkeley
Berkeley, United States
28 h-index
51 publications
10.8K citations

Space Telescope Science Institute
Baltimore, United States
26 h-index
37 publications
4.8K citations
Carnegie Observatories
Pasadena, United States
24 h-index
61 publications
14.3K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
23 h-index
51 publications
7.7K citations
University of Arizona
Tucson, United States
22 h-index
48 publications
6.1K citations
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ApJ · 294 publications · 37.2K citations
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163 publications · 15.5K citations
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AJ · 71 publications · 6.2K citations
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67 publications · 5.2K citations
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Repository · 16 publications · 1.2K citations
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