Galaxy Morphology Evolution

Galaxy Morphology Evolution is a theoretical construct in astrophysics that characterizes the transformation over cosmic time in the structural forms of galaxies, such as their shape, size, and component distribution, as driven by internal processes and external interactions within the broader framework of galaxy formation and evolution.

643

Publications

59.1K

Citations

2.6K

Authors

647

Institutions

Publications per year

2017–2026

185

Authors

2.6K

  1. AM
    Anton M. Koekemoer

    Space Telescope Science Institute, United States

    17 publications · 1.6K citations

    17

    h-index

  2. SF
    S. F. Sánchez

    Universidad Nacional Autónoma de México, Mexico

    17 publications · 3.6K citations

    15

    h-index

  3. LP
    L. Pozzetti

    University of Bologna, Italy

    13 publications · 1.5K citations

    13

    h-index

  4. LW
    L. Wisotzki

    Leibniz Institute for Astrophysics Potsdam, Germany

    12 publications · 3.4K citations

    12

    h-index

  5. GZ
    G. Zamorani

    University of Bologna, Italy

    13 publications · 1.2K citations

    12

    h-index

1–5 of 2.6K

Venues

  1. The Astrophysical Journal

    ApJ · 133 publications · 15.7K citations

    60

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    180 publications · 13.6K citations

    59

    h-index

  3. Astronomy and Astrophysics

    89 publications · 6.4K citations

    40

    h-index

  4. The Astronomical Journal

    AJ · 33 publications · 1.8K citations

    23

    h-index

  5. arXiv (Cornell University)

    Repository · 14 publications · 711 citations

    13

    h-index

1–5