Spiral Density Waves

Spiral Density Waves is a theoretical construct in galactic dynamics that models the spiral structure of disk galaxies as Quasi-stationary, large-scale patterns of enhanced mass density propagating through the stellar disk, where gravitational instabilities sustain coherent waveforms that rotate rigidly while perturbing stellar and gas orbits without requiring material arms.

444

Publications

26K

Citations

934

Authors

428

Institutions

Publications per year

2017–2026

60

Authors

934

  1. BG
    Bruce G. Elmegreen

    IBM (United States), United States

    17 publications · 1.4K citations

    15

    h-index

  2. FH
    Frank H. Shu

    University of California, Berkeley, United States

    14 publications · 1.8K citations

    13

    h-index

  3. DM
    D. M. Elmegreen

    Vassar College, United States

    10 publications · 859 citations

    10

    h-index

  4. CY
    Chi Yuan

    Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan

    10 publications · 298 citations

    10

    h-index

  5. EG
    Evgeny Griv

    Ben-Gurion University of the Negev, Israel

    9 publications · 176 citations

    9

    h-index

1–5 of 934

Venues

  1. The Astrophysical Journal

    ApJ · 154 publications · 11.6K citations

    61

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    92 publications · 4.1K citations

    34

    h-index

  3. Astronomy and Astrophysics

    27 publications · 1.2K citations

    21

    h-index

  4. The Astronomical Journal

    AJ · 24 publications · 1.3K citations

    19

    h-index

  5. The Astrophysical Journal Letters

    12 publications · 1.3K citations

    12

    h-index

1–5