Galactic Shear

Galactic Shear is a kinematic phenomenon in galactic dynamics characterized by the differential rotation of adjacent regions of a galaxy, where the relative motion of stars or gas clouds results in a velocity gradient across a given radial distance from the galactic center.

88

Publications

7.5K

Citations

288

Authors

194

Institutions

Publications per year

2017–2026

21

Variants

Galactic Differential Rotation

Authors

288

  1. PS
    Peter Schneider

    University of Bonn, Germany

    4 publications · 105 citations

    4

    h-index

  2. MR
    Mark R. Krumholz

    Australian National University, Australia

    3 publications · 229 citations

    3

    h-index

  3. BG
    Bruce G. Elmegreen

    IBM (United States), United States

    3 publications · 150 citations

    3

    h-index

  4. JM
    J. M. Diederik Kruijssen

    Heidelberg University, Germany

    3 publications · 215 citations

    3

    h-index

  5. HH
    Henk Hoekstra

    Leiden University, Netherlands

    3 publications · 715 citations

    3

    h-index

1–5 of 288

Venues

  1. Monthly Notices of the Royal Astronomical Society

    29 publications · 3.7K citations

    24

    h-index

  2. The Astrophysical Journal

    ApJ · 22 publications · 1.4K citations

    21

    h-index

  3. Astronomy and Astrophysics

    9 publications · 426 citations

    9

    h-index

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

    Repository · 4 publications · 481 citations

    4

    h-index

  5. The Astronomical Journal

    AJ · 3 publications · 168 citations

    3

    h-index

1–5