Swing Amplification

Swing Amplification is a theoretical mechanism in galactic dynamics that explains the transient growth of spiral density waves in differentially rotating stellar disks through the coherent alignment of leading and trailing perturbations, enhanced by self-gravity and shear.

36

Publications

1.7K

Citations

51

Authors

44

Institutions

Publications per year

2017–2026

6

Authors

51

  1. BF
    B. Fuchs

    Heidelberg University, Germany

    5 publications · 124 citations

    5

    h-index

  2. CP
    Christophe Pichon

    Institut d'Astrophysique de Paris, France

    3 publications · 95 citations

    3

    h-index

  3. JF
    Jean-Baptiste Fouvry

    Centre National de la Recherche Scientifique, France

    3 publications · 95 citations

    3

    h-index

  4. JB
    Junichi Baba

    National Astronomical Observatory of Japan, Japan

    2 publications · 126 citations

    2

    h-index

  5. TT
    T. Tsuchiya

    National Institute of Advanced Industrial Science and Technology, Japan

    2 publications · 32 citations

    2

    h-index

1–5 of 51

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 868 citations

    13

    h-index

  2. 12

    h-index

  3. Astronomy and Astrophysics

    5 publications · 162 citations

    5

    h-index

  4. ArXiv.org

    Repository · 2 publications · 38 citations

    2

    h-index

  5. The Astrophysical Journal Letters

    1 publications · 41 citations

    1

    h-index

1–5