Surface Gravity Classification

Surface Gravity Classification is a stellar classification method that categorizes stars based on their surface gravity, typically derived from spectral line sensitivity to gravitational pressure, thereby distinguishing stellar evolutionary stages such as dwarfs, giants, and supergiants within the broader system of stellar spectral taxonomy.

7

Publications

661

Citations

26

Authors

29

Institutions

Publications per year

2017–2026

2

Variants

Luminosity Class

Authors

26

  1. EL
    Emily L. Rice

    American Museum of Natural History, United States

    2 publications · 328 citations

    2

    h-index

  2. JG
    Jonathan Gagné

    Université de Montréal, Canada

    1 publications · 264 citations

    1

    h-index

  3. JK
    Jacqueline K. Faherty

    American Museum of Natural History, United States

    1 publications · 264 citations

    1

    h-index

  4. VB
    Vivienne Baldassare

    University of Michigan, United States

    1 publications · 264 citations

    1

    h-index

  5. JR
    J. R. Thorstensen

    Dartmouth College, United States

    1 publications · 264 citations

    1

    h-index

1–5 of 26

Venues

  1. The Astrophysical Journal

    ApJ · 3 publications · 166 citations

    3

    h-index

  2. The Astrophysical Journal Letters

    1 publications · 162 citations

    1

    h-index

  3. The Astrophysical Journal Supplement Series

    1 publications · 264 citations

    1

    h-index

  4. The Astronomical Journal

    AJ · 1 publications · 41 citations

    1

    h-index

  5. Journal of Geodesy

    1 publications · 28 citations

    1

    h-index

1–5