Bulge Density Profiles

Bulge Density Profiles is a theoretical astrophysical model that characterizes the spatial distribution of stellar mass within the central region of a galaxy by specifying how density varies with distance from the galactic center, distinguishing it from disk or halo density models through its focus on the spheroidal bulge component.

62

Publications

6.1K

Citations

132

Authors

109

Institutions

Publications per year

2017–2026

12

Authors

132

  1. OG
    Ortwin Gerhard

    Max Planck Institute for Extraterrestrial Physics, Germany

    7 publications · 1.1K citations

    7

    h-index

  2. MZ
    M. Zoccali

    Pontificia Universidad Católica de Chile, Chile

    4 publications · 263 citations

    4

    h-index

  3. OA
    O. A. González

    Pontificia Universidad Católica de Chile, Chile

    4 publications · 263 citations

    4

    h-index

  4. EV
    E. Valenti

    European Southern Observatory, Germany

    3 publications · 165 citations

    3

    h-index

  5. DM
    D. Minniti

    Pontificia Universidad Católica de Chile, Chile

    3 publications · 244 citations

    3

    h-index

1–5 of 132

Venues

  1. Monthly Notices of the Royal Astronomical Society

    21 publications · 3.6K citations

    19

    h-index

  2. The Astrophysical Journal

    ApJ · 8 publications · 822 citations

    8

    h-index

  3. Astronomy and Astrophysics

    7 publications · 348 citations

    7

    h-index

  4. CERN Document Server (European Organization for Nuclear Research)

    Repository · 3 publications · 374 citations

    3

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 3 publications · 49 citations

    3

    h-index

1–5