Stellar Luminosity Evolution

Stellar Luminosity Evolution is the time-dependent change in a star's total electromagnetic energy output per unit time, distinguishing it from static luminosity measures by characterizing how stellar brightness varies across its evolutionary phases due to internal structural and compositional changes.

286

Publications

29.9K

Citations

1.1K

Authors

389

Institutions

Publications per year

2017–2026

33

Authors

1.1K

  1. JR
    J. R. Mould

    California Institute of Technology, United States

    4 publications · 122 citations

    4

    h-index

  2. AV
    A. V. Sweigart

    Goddard Space Flight Center, United States

    4 publications · 514 citations

    4

    h-index

  3. CA
    Christopher A. Tout

    Institute of Astronomy, Russia

    4 publications · 2.7K citations

    4

    h-index

  4. GD
    G. D. Illingworth

    University of California, Santa Cruz, United States

    3 publications · 366 citations

    3

    h-index

  5. GH
    G. H. Rieke

    University of Arizona, United States

    3 publications · 84 citations

    3

    h-index

1–5 of 1.1K

Venues

  1. The Astrophysical Journal

    ApJ · 146 publications · 14.1K citations

    59

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    46 publications · 6.9K citations

    29

    h-index

  3. Astronomy and Astrophysics

    22 publications · 1.4K citations

    17

    h-index

  4. The Astronomical Journal

    AJ · 12 publications · 682 citations

    11

    h-index

  5. The Astrophysical Journal Supplement Series

    10 publications · 2.6K citations

    10

    h-index

1–5