Pre-main-sequence Variables

Pre-Main-Sequence Variables is a class of variable stars comprising young stellar objects in the early evolutionary phase preceding the main sequence, distinguished by irregular photometric variability due to accretion processes, circumstellar disk interactions, and magnetic activity rather than stable hydrogen fusion.

78

Publications

4.4K

Citations

239

Authors

150

Institutions

Publications per year

2017–2026

11

Authors

239

  1. WH
    W. Herbst

    Wesleyan University, United States

    4 publications · 274 citations

    4

    h-index

  2. RM
    R. Mundt

    Max Planck Institute for Astronomy, Germany

    4 publications · 273 citations

    4

    h-index

  3. PG
    P. G. Prada Moroni

    University of Pisa, Italy

    3 publications · 127 citations

    3

    h-index

  4. JC
    J. C. Pandey

    Aryabhatta Research Institute of Observational Sciences, India

    3 publications · 50 citations

    3

    h-index

  5. AK
    A. K. Pandey

    Aryabhatta Research Institute of Observational Sciences, India

    3 publications · 46 citations

    3

    h-index

1–5 of 239

Venues

  1. 13

    h-index

  2. The Astrophysical Journal

    ApJ · 11 publications · 698 citations

    12

    h-index

  3. Astronomy and Astrophysics

    13 publications · 633 citations

    12

    h-index

  4. The Astronomical Journal

    AJ · 10 publications · 488 citations

    10

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 53 citations

    4

    h-index

1–5