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.

790

Publications

79.4K

Citations

5.1K

Authors

713

Institutions

Publications per year

2017–2026

114

Variants

Mass-luminosity Relationship

Authors

5.1K

  1. MM
    M. Marconi

    Astronomical Observatory of Capodimonte, Italy

    10 publications · 405 citations

    10

    h-index

  2. TT
    Tommaso Treu

    University of California, Los Angeles, United States

    9 publications · 943 citations

    9

    h-index

  3. HB
    H. Böhringer

    Max Planck Institute for Extraterrestrial Physics, Germany

    8 publications · 948 citations

    8

    h-index

  4. IM
    I. Musella

    Astronomical Observatory of Capodimonte, Italy

    8 publications · 272 citations

    8

    h-index

  5. NM
    N. Morrell

    Las Campanas Observatory, Chile

    7 publications · 432 citations

    7

    h-index

1–5 of 5.1K

Venues

  1. The Astrophysical Journal

    ApJ · 294 publications · 37.2K citations

    84

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    163 publications · 15.5K citations

    57

    h-index

  3. The Astronomical Journal

    AJ · 71 publications · 6.2K citations

    36

    h-index

  4. Astronomy and Astrophysics

    67 publications · 5.2K citations

    35

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 16 publications · 1.2K citations

    15

    h-index

1–5