Cluster Substructure

Cluster Substructure is a morphological construct in astrophysics that denotes statistically significant deviations from smooth, centrally symmetric spatial distributions of galaxies or stellar systems within a cluster, indicating hierarchical assembly, recent mergers, or dynamical youth.

171

Publications

11.4K

Citations

580

Authors

291

Institutions

Publications per year

2017–2026

20

Authors

580

  1. GP
    G. P. Smith

    University of Birmingham, United Kingdom

    9 publications · 739 citations

    9

    h-index

  2. HB
    H. Böhringer

    Max Planck Institute for Extraterrestrial Physics, Germany

    6 publications · 323 citations

    6

    h-index

  3. AB
    A. Biviano

    Trieste Astronomical Observatory, Italy

    5 publications · 284 citations

    5

    h-index

  4. EE
    Eiichi Egami

    University of Arizona, United States

    5 publications · 336 citations

    5

    h-index

  5. MJ
    Michael J. West

    University of Hawaii at Hilo, United States

    4 publications · 336 citations

    4

    h-index

1–5 of 580

Venues

  1. 29

    h-index

  2. The Astrophysical Journal

    ApJ · 29 publications · 1.8K citations

    23

    h-index

  3. Astronomy and Astrophysics

    21 publications · 1.4K citations

    18

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 940 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 78 citations

    4

    h-index

1–5