Early Stellar Variability

Early Stellar Variability is a theoretical construct in pre-main-sequence evolution that characterizes the intrinsic fluctuations in luminosity and spectral properties of young stellar objects arising from accretion processes, rotation, and circumstellar disk interactions during the early phases of stellar development.

45

Publications

2.8K

Citations

188

Authors

113

Institutions

Publications per year

2017–2026

4

Authors

188

  1. WH
    W. Herbst

    Wesleyan University, United States

    3 publications · 378 citations

    3

    h-index

  2. JB
    J. Bouvier

    Centre National de la Recherche Scientifique, France

    3 publications · 407 citations

    3

    h-index

  3. JF
    J. Fabregat

    Universitat de València, Spain

    2 publications · 255 citations

    2

    h-index

  4. SM
    S. Melnikov

    Academy of Sciences Republic of Uzbekistan, Uzbekistan

    2 publications · 334 citations

    2

    h-index

  5. RK
    R. K. Prinja

    University College London, United Kingdom

    2 publications · 90 citations

    2

    h-index

1–5 of 188

Venues

  1. The Astrophysical Journal

    ApJ · 11 publications · 1K citations

    11

    h-index

  2. 10

    h-index

  3. Astronomy and Astrophysics

    5 publications · 384 citations

    5

    h-index

  4. Astrophysics and Space Science

    3 publications · 46 citations

    4

    h-index

  5. The Astronomical Journal

    AJ · 3 publications · 254 citations

    3

    h-index

1–5