Bar-driven Spiral Structure

Bar-Driven Spiral Structure is a theoretical astrophysical model within galactic dynamics that specifies spiral arm formation in disk galaxies as primarily induced and sustained by non-axisymmetric gravitational perturbations originating from a central stellar bar.

57

Publications

3.8K

Citations

160

Authors

131

Institutions

Publications per year

2017–2026

7

Authors

160

  1. JH
    J. H. Knapen

    Instituto de Astrofísica de Canarias, Spain

    4 publications · 267 citations

    4

    h-index

  2. EL
    E. Laurikainen

    University of Oulu, Finland

    3 publications · 201 citations

    3

    h-index

  3. FC
    F. Combes

    Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères, France

    3 publications · 191 citations

    3

    h-index

  4. HS
    H. Salo

    University of Oulu, Finland

    3 publications · 201 citations

    3

    h-index

  5. LA
    L. A. Martinez-Medina

    Universidad Nacional Autónoma de México, Mexico

    2 publications · 32 citations

    2

    h-index

1–5 of 160

Venues

  1. Monthly Notices of the Royal Astronomical Society

    19 publications · 1.4K citations

    18

    h-index

  2. The Astrophysical Journal

    ApJ · 16 publications · 1.1K citations

    14

    h-index

  3. Astronomy and Astrophysics

    5 publications · 369 citations

    5

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 208 citations

    4

    h-index

  5. The Astrophysical Journal Letters

    2 publications · 107 citations

    2

    h-index

1–5