Stellar Evolutionary States

Stellar Evolutionary States is a theoretical construct that categorizes the distinct phases of a star's life cycle, such as pre-main sequence, main sequence, red giant, and white dwarf, based on its physical properties and nuclear fusion processes, thereby distinguishing it from other stellar classification schemes by focusing on temporal development and energy generation mechanisms.

345

Publications

26.4K

Citations

1.2K

Authors

469

Institutions

Publications per year

2017–2026

64

Variants

Stellar Evolutionary Phases

Authors

1.2K

  1. YE
    Y. Elsworth

    University of Birmingham, United Kingdom

    8 publications · 746 citations

    8

    h-index

  2. JV
    J. V. Clausen

    University of Copenhagen, Denmark

    6 publications · 192 citations

    6

    h-index

  3. GG
    G. Gilmore

    University of Cambridge, United Kingdom

    6 publications · 439 citations

    6

    h-index

  4. SH
    S. Hekker

    Aarhus University, Denmark

    6 publications · 579 citations

    6

    h-index

  5. BA
    B. A. Wilking

    University of Missouri–St. Louis, United States

    6 publications · 222 citations

    6

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 90 publications · 6.5K citations

    44

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    55 publications · 2.3K citations

    32

    h-index

  3. Astronomy and Astrophysics

    62 publications · 3K citations

    32

    h-index

  4. The Astronomical Journal

    AJ · 27 publications · 1.9K citations

    24

    h-index

  5. The Astrophysical Journal Letters

    11 publications · 700 citations

    11

    h-index

1–5