Classical Bulge

Classical Bulge is a structural component of a galaxy characterized by a dense, pressure-supported stellar population that exhibits little to no rotational support and forms through rapid, early hierarchical merging processes distinct from secular evolution.

134

Publications

10.7K

Citations

366

Authors

229

Institutions

Publications per year

2017–2026

45

Variants

Classical Galactic Bulge

Authors

366

  1. RP
    R. P. Saglia

    Max Planck Institute for Extraterrestrial Physics, Germany

    8 publications · 736 citations

    8

    h-index

  2. RB
    R. Bender

    Max Planck Institute for Extraterrestrial Physics, Germany

    8 publications · 736 citations

    8

    h-index

  3. PE
    Peter Erwin

    Max Planck Institute for Extraterrestrial Physics, Germany

    7 publications · 648 citations

    7

    h-index

  4. AB
    A. Boselli

    Laboratoire d’Astrophysique de Marseille, France

    7 publications · 476 citations

    7

    h-index

  5. MF
    Michele Fumagalli

    Durham University, United Kingdom

    7 publications · 476 citations

    7

    h-index

1–5 of 366

Venues

  1. Monthly Notices of the Royal Astronomical Society

    52 publications · 3.9K citations

    31

    h-index

  2. The Astrophysical Journal

    ApJ · 27 publications · 2.4K citations

    22

    h-index

  3. Astronomy and Astrophysics

    18 publications · 1.4K citations

    17

    h-index

  4. The Astrophysical Journal Letters

    10 publications · 904 citations

    10

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 5 publications · 286 citations

    5

    h-index

1–5