Stellar Contraction Tracks

Stellar Contraction Tracks is a theoretical construct in stellar astrophysics that represents the evolutionary paths of pre-main-sequence stars in the Hertzsprung-Russell diagram as they gravitationally contract toward the zero-age main sequence, distinguished from other evolutionary tracks by their dependence on initial mass, angular momentum, and accretion history during the contraction phase.

7

Publications

618

Citations

52

Authors

33

Institutions

Publications per year

2017–2026

1

Authors

52

  1. AR
    A. Reiners

    University of Göttingen, Germany

    1 publications · 71 citations

    1

    h-index

  2. EG
    E. González-Álvarez

    Osservatorio Astrofisico di Torino, Italy

    1 publications · 71 citations

    1

    h-index

  3. JA
    J. A. Caballero

    Centro de Astrobiología, Spain

    1 publications · 71 citations

    1

    h-index

  4. HC
    H. C. P.

    1 publications · 84 citations

    1

    h-index

  5. NL
    N. Lodieu

    Instituto de Astrofísica de Canarias, Spain

    1 publications · 71 citations

    1

    h-index

1–5 of 52

Venues

  1. 2

    h-index

  2. The Astrophysical Journal

    ApJ · 2 publications · 246 citations

    2

    h-index

  3. 1

    h-index

  4. Nature Astronomy

    1 publications · 71 citations

    1

    h-index

  5. Nature

    1 publications · 84 citations

    1

    h-index

1–5