Galaxy Nucleus Classification

Galaxy Nucleus Classification is a systematic framework in astrophysics that categorizes galactic nuclei based on their observational and physical properties, distinguishing them according to the dominant energy source, spectral characteristics, and morphological features indicative of active galactic nuclei, starburst activity, or quiescent states.

37

Publications

1.4K

Citations

119

Authors

106

Institutions

Publications per year

2017–2026

7

Authors

119

  1. JL
    J. L. Sérsic

    Argentine National Observatory, Argentina

    3 publications · 252 citations

    3

    h-index

  2. LV
    L. Verdes‐Montenegro

    Instituto de Astrofísica de Andalucía, Spain

    2 publications · 44 citations

    2

    h-index

  3. MG
    M. G. Pastoriza

    Universidade Federal do Rio Grande do Sul, Brazil

    2 publications · 217 citations

    2

    h-index

  4. GS
    G. Savorgnan

    Swinburne University of Technology, Australia

    2 publications · 44 citations

    2

    h-index

  5. SG
    S. García‐Burillo

    Spanish National Observatory, Spain

    2 publications · 73 citations

    2

    h-index

1–5 of 119

Venues

  1. The Astrophysical Journal

    ApJ · 6 publications · 197 citations

    6

    h-index

  2. Astronomy and Astrophysics

    5 publications · 190 citations

    5

    h-index

  3. Publications of the Astronomical Society of the Pacific

    PASP · 5 publications · 359 citations

    5

    h-index

  4. The Astronomical Journal

    AJ · 3 publications · 148 citations

    3

    h-index

  5. 3

    h-index

1–5