Stellar Spectral Classification

Stellar Spectral Classification is a systematic astrophysical framework that categorizes stars based on their electromagnetic spectra, particularly the patterns of absorption lines, to infer fundamental physical properties such as temperature, luminosity, and chemical composition.

1.3K

Publications

93.8K

Citations

3.5K

Authors

821

Institutions

Publications per year

2017–2026

183

Authors

3.5K

  1. NR
    N. R. Walborn

    Space Telescope Science Institute, United States

    30 publications · 3.9K citations

    26

    h-index

  2. AL
    A-Li Luo

    National Astronomical Observatories, China

    22 publications · 711 citations

    19

    h-index

  3. RO
    R. O. Gray

    Appalachian State University, United States

    19 publications · 2.9K citations

    18

    h-index

  4. HA
    Helmut A. Abt

    Kitt Peak National Observatory, United States

    22 publications · 1.4K citations

    16

    h-index

  5. PC
    Philip C. Keenan

    The Ohio State University, United States

    18 publications · 1.7K citations

    16

    h-index

1–5 of 3.5K

Venues

  1. The Astrophysical Journal

    ApJ · 298 publications · 20.8K citations

    74

    h-index

  2. The Astronomical Journal

    AJ · 170 publications · 18.4K citations

    60

    h-index

  3. The Astrophysical Journal Supplement Series

    115 publications · 18.2K citations

    57

    h-index

  4. Astronomy and Astrophysics

    158 publications · 9.2K citations

    51

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    167 publications · 8.2K citations

    46

    h-index

1–5