Boxy Bulge

Boxy Bulge is a type of galactic bulge morphology distinguished by its triaxial, rectangular-like shape observed in edge-on disk galaxies, resulting from the secular evolution of the galactic bar and resonant stellar orbits.

114

Publications

9.6K

Citations

239

Authors

193

Institutions

Publications per year

2017–2026

33

Variants

Boxy-peanut BulgeBoxy/peanut-shaped Bulge

Authors

239

  1. EA
    E. Athanassoula

    Centre National de la Recherche Scientifique, France

    14 publications · 1.8K citations

    14

    h-index

  2. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    12 publications · 2.7K citations

    12

    h-index

  3. VP
    Victor P. Debattista

    University of Lancashire, United Kingdom

    10 publications · 562 citations

    10

    h-index

  4. MB
    Martin Bureau

    University of Oxford, United Kingdom

    8 publications · 688 citations

    8

    h-index

  5. PD
    P. Di Matteo

    Galaxies, Etoiles, Physique et Instrumentation, France

    7 publications · 298 citations

    7

    h-index

1–5 of 239

Venues

  1. Monthly Notices of the Royal Astronomical Society

    41 publications · 3.4K citations

    31

    h-index

  2. Astronomy and Astrophysics

    14 publications · 937 citations

    13

    h-index

  3. The Astrophysical Journal

    ApJ · 10 publications · 614 citations

    10

    h-index

  4. The Astrophysical Journal Letters

    10 publications · 886 citations

    10

    h-index

  5. 5

    h-index

1–5