Hayashi Track

A "Hayashi Track" is a theoretical evolutionary path in the Hertzsprung-Russell diagram that describes the nearly vertical contraction phase of pre-main-sequence stars, characterized by fully convective interiors and constant effective temperature, as they gravitationally contract toward the main sequence.

49

Publications

5K

Citations

134

Authors

82

Institutions

Publications per year

2017–2026

4

Authors

134

  1. AW
    Aneta Wojnar

    Universidad Complutense de Madrid, Spain

    3 publications · 56 citations

    3

    h-index

  2. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 341 citations

    3

    h-index

  3. SJ
    Scott J. Kenyon

    Smithsonian Astrophysical Observatory, United States

    2 publications · 139 citations

    2

    h-index

  4. TP
    Thomas P. Greene

    Ames Research Center, United States

    2 publications · 160 citations

    2

    h-index

  5. RD
    R. D. Jeffries

    Keele University, United Kingdom

    2 publications · 96 citations

    2

    h-index

1–5 of 134

Venues

  1. The Astrophysical Journal

    ApJ · 23 publications · 2K citations

    20

    h-index

  2. 7

    h-index

  3. Astronomy and Astrophysics

    4 publications · 215 citations

    4

    h-index

  4. The Astronomical Journal

    AJ · 3 publications · 376 citations

    3

    h-index

  5. The Astrophysical Journal Letters

    1 publications · 17 citations

    1

    h-index

1–5