Multi-arm Spiral Patterns

Multi-Arm Spiral Patterns is a theoretical construct in galactic astronomy that describes the coherent, large-scale organization of spiral density waves in disk galaxies characterized by the presence of two or more dominant spiral arms originating from the galactic center, distinguishing it from single-arm or flocculent spiral configurations by its higher symmetry and arm multiplicity.

39

Publications

1.9K

Citations

96

Authors

58

Institutions

Publications per year

2017–2026

4

Authors

96

  1. PD
    P. D. Nicholson

    Cornell University, United States

    2 publications · 121 citations

    2

    h-index

  2. MM
    Matthew M. Hedman

    Cornell University, United States

    2 publications · 121 citations

    2

    h-index

  3. JP
    J. P. Vallée

    Herzberg Institute of Astrophysics, Canada

    2 publications · 140 citations

    2

    h-index

  4. JE
    J. Eder

    Cornell University, United States

    1 publications · 44 citations

    1

    h-index

  5. YX
    Ye Xu

    Purple Mountain Observatory, China

    1 publications · 41 citations

    1

    h-index

1–5 of 96

Venues

  1. The Astrophysical Journal

    ApJ · 11 publications · 710 citations

    11

    h-index

  2. 7

    h-index

  3. The Astronomical Journal

    AJ · 5 publications · 321 citations

    5

    h-index

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

    Repository · 1 publications · 18 citations

    1

    h-index

  5. Communications in Theoretical Physics

    CTP · 1 publications · 10 citations

    1

    h-index

1–5