Concepedia

Henyey Track

A Henyey Track is a theoretical evolutionary path in the Hertzsprung-Russell diagram that describes the quasi-static contraction phase of pre-main-sequence stars, distinguishing itself from other pre-main-sequence tracks by modeling stars with substantial radiative interiors and minimal surface convection during late-stage gravitational contraction prior to reaching the main sequence.

3

Publications

84

Citations

4

Authors

4

Institutions

Publications per year

2017–2026

1

Parents

Publications

3

1–3 of 3

Authors

4

  1. CL
    Claire L. Davies

    University of Exeter, United Kingdom

    1 publications · 30 citations

    1

    h-index

  2. SJ
    Stephen Jackson

    NSF NCAR High Altitude Observatory, United States

    1 publications · 24 citations

    1

    h-index

  3. SG
    S. G. Gregory

    University of St Andrews, United Kingdom

    1 publications · 30 citations

    1

    h-index

  4. FC
    Fred C. Adams

    University of Michigan, United States

    1 publications · 30 citations

    1

    h-index

1–4 of 4

Institutions

4

  1. The University of Texas at Austin

    Austin, United States

    1 h-index

    1 publications

    30 citations

  2. University of St Andrews

    St Andrews, United Kingdom

    1 h-index

    2 publications

    60 citations

  3. University of Exeter

    Exeter, United Kingdom

    1 h-index

    1 publications

    30 citations

  4. University of Michigan

    Ann Arbor, United States

    1 h-index

    1 publications

    30 citations

1–4 of 4

Venues

  1. The Astrophysical Journal

    ApJ · 2 publications · 54 citations

    2

    h-index

  2. 1

    h-index

1–2