Galactic Mass Distribution

Galactic Mass Distribution is a theoretical construct in astrophysics that specifies the spatial arrangement of stellar, gaseous, dark matter, and total mass components within a galaxy as a function of radius, enabling the modeling of gravitational potentials and rotational dynamics.

779

Publications

71.7K

Citations

1.9K

Authors

602

Institutions

Publications per year

2017–2026

136

Authors

1.9K

  1. CS
    Carlos S. Frenk

    Durham University, United Kingdom

    13 publications · 2.5K citations

    13

    h-index

  2. PJ
    P. J. E. Peebles

    Princeton University, United States

    12 publications · 799 citations

    11

    h-index

  3. OB
    O. Bienaymé

    Observatoire astronomique de Strasbourg, France

    11 publications · 973 citations

    11

    h-index

  4. LH
    Lars Hernquist

    Center for Astrophysics Harvard & Smithsonian, United States

    11 publications · 2.4K citations

    11

    h-index

  5. JB
    Joss Bland‐Hawthorn

    The University of Sydney, Australia

    9 publications · 568 citations

    9

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 269 publications · 28.1K citations

    88

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    169 publications · 20.2K citations

    64

    h-index

  3. The Astronomical Journal

    AJ · 52 publications · 3.5K citations

    34

    h-index

  4. Astronomy and Astrophysics

    48 publications · 3.9K citations

    33

    h-index

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

    Repository · 14 publications · 600 citations

    13

    h-index

1–5