Protostellar Luminosity Evolution

Protostellar Luminosity Evolution is a theoretical construct in astrophysics that models the temporal changes in electromagnetic energy output of a protostar as it gravitationally contracts toward the zero-age main sequence, distinguishing itself by integrating accretion history, mass-loss processes, and stellar structural development over time.

18

Publications

1.3K

Citations

55

Authors

64

Institutions

Publications per year

2017–2026

1

Authors

55

  1. AS
    A. Schmiedeke

    University of Cologne, Germany

    2 publications · 39 citations

    2

    h-index

  2. AZ
    A. Zernickel

    University of Cologne, Germany

    2 publications · 39 citations

    2

    h-index

  3. GS
    G. Stéphan

    University of Cologne, Germany

    2 publications · 39 citations

    2

    h-index

  4. TM
    T. Möller

    University of Cologne, Germany

    2 publications · 39 citations

    2

    h-index

  5. PS
    P. Schilke

    Max Planck Institute for Radio Astronomy, Germany

    2 publications · 39 citations

    2

    h-index

1–5 of 55

Venues

  1. The Astrophysical Journal

    ApJ · 6 publications · 786 citations

    5

    h-index

  2. 3

    h-index

  3. Astronomy and Astrophysics

    2 publications · 45 citations

    2

    h-index

  4. The Astronomical Journal

    AJ · 1 publications · 53 citations

    1

    h-index

  5. Kölner Universitäts PublikationsServer (Universität zu Köln)

    Repository · 1 publications · 13 citations

    1

    h-index

1–5