Bulge Structure

Bulge Structure is a structural component of a galaxy characterized as a dense, centrally concentrated stellar population that distinguishes itself from the disk and halo components by its distinct kinematic, photometric, and metallicity properties.

513

Publications

46.5K

Citations

1.5K

Authors

564

Institutions

Publications per year

2017–2026

104

Authors

1.5K

  1. EM
    E. M. Corsini

    University of Padua, Italy

    13 publications · 717 citations

    13

    h-index

  2. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    13 publications · 2K citations

    13

    h-index

  3. AW
    Alister W. Graham

    Swinburne University of Technology, Australia

    11 publications · 872 citations

    11

    h-index

  4. MB
    M. Balcells

    Instituto de Astrofísica de Canarias, Spain

    12 publications · 1.3K citations

    11

    h-index

  5. JM
    J. Méndez‐Abreu

    Instituto de Astrofísica de Canarias, Spain

    11 publications · 479 citations

    11

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 97 publications · 13.9K citations

    52

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    101 publications · 9.3K citations

    47

    h-index

  3. Astronomy and Astrophysics

    47 publications · 5.1K citations

    31

    h-index

  4. The Astronomical Journal

    AJ · 38 publications · 2.9K citations

    26

    h-index

  5. Nucleic Acids Research

    13 publications · 478 citations

    13

    h-index

1–5