Bulge Morphology

Bulge Morphology is a structural characterization framework that describes the geometric and photometric properties of the central stellar population in galaxies, specifically distinguishing the Milky Way's bulge component by its three-dimensional shape, stellar density distribution, and kinematic features relative to the disk and halo.

443

Publications

41.5K

Citations

1.2K

Authors

506

Institutions

Publications per year

2017–2026

76

Authors

1.2K

  1. JM
    J. Méndez‐Abreu

    Instituto de Astrofísica de Canarias, Spain

    11 publications · 437 citations

    11

    h-index

  2. MB
    M. Balcells

    Instituto de Astrofísica de Canarias, Spain

    11 publications · 1K citations

    10

    h-index

  3. EM
    E. M. Corsini

    University of Padua, Italy

    9 publications · 492 citations

    9

    h-index

  4. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    9 publications · 1.4K citations

    9

    h-index

  5. AW
    Alister W. Graham

    Swinburne University of Technology, Australia

    8 publications · 667 citations

    8

    h-index

1–5 of 1.2K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    90 publications · 8.4K citations

    50

    h-index

  2. The Astrophysical Journal

    ApJ · 73 publications · 11.8K citations

    44

    h-index

  3. The Astronomical Journal

    AJ · 36 publications · 2.4K citations

    27

    h-index

  4. Astronomy and Astrophysics

    32 publications · 2.2K citations

    23

    h-index

  5. The Astrophysical Journal Supplement Series

    6 publications · 1.8K citations

    7

    h-index

1–5