Arm Interarm Contrast

Arm Interarm Contrast is a quantitative metric in galactic astronomy that measures the relative density or brightness difference between the spiral arms and the interarm regions of a galaxy, thereby characterizing the prominence of spiral structure in the context of Milky Way Structure.

35

Publications

2.5K

Citations

130

Authors

84

Institutions

Publications per year

2017–2026

3

Authors

130

  1. DM
    D. M. Elmegreen

    Vassar College, United States

    4 publications · 308 citations

    4

    h-index

  2. JH
    J. H. Knapen

    Instituto de Astrofísica de Canarias, Spain

    3 publications · 200 citations

    3

    h-index

  3. RB
    R. Buta

    University of Alabama, United States

    2 publications · 190 citations

    2

    h-index

  4. MW
    Michael W. Regan

    Space Telescope Science Institute, United States

    2 publications · 174 citations

    2

    h-index

  5. NK
    Nario Kuno

    National Astronomical Observatory of Japan, Japan

    2 publications · 43 citations

    2

    h-index

1–5 of 130

Venues

  1. The Astrophysical Journal

    ApJ · 10 publications · 580 citations

    11

    h-index

  2. The Astronomical Journal

    AJ · 5 publications · 231 citations

    5

    h-index

  3. 4

    h-index

  4. The Astrophysical Journal Letters

    3 publications · 289 citations

    3

    h-index

  5. Astronomy and Astrophysics

    3 publications · 186 citations

    3

    h-index

1–5