Disk Star Formation Differences

Disk Star Formation Differences is a theoretical construct that characterizes variations in star formation rates, efficiencies, and modes across different galactic disk environments, distinguishing itself by focusing on the physical and structural disparities within rotating disk galaxies rather than global or extragalactic contexts.

34

Publications

2.8K

Citations

191

Authors

122

Institutions

Publications per year

2017–2026

5

Authors

191

  1. JH
    J. H. Knapen

    Instituto de Astrofísica de Canarias, Spain

    4 publications · 267 citations

    4

    h-index

  2. RA
    Rebecca A. Koopmann

    Union College, United States

    3 publications · 314 citations

    3

    h-index

  3. PA
    P. A. James

    Liverpool John Moores University, United Kingdom

    3 publications · 155 citations

    3

    h-index

  4. BC
    Barbara Catinella

    International Centre for Radio Astronomy Research, Australia

    2 publications · 169 citations

    2

    h-index

  5. SM
    S. M. Percival

    Liverpool John Moores University, United Kingdom

    2 publications · 118 citations

    2

    h-index

1–5 of 191

Venues

  1. The Astrophysical Journal

    ApJ · 14 publications · 1K citations

    14

    h-index

  2. Astronomy and Astrophysics

    5 publications · 389 citations

    5

    h-index

  3. The Astronomical Journal

    AJ · 5 publications · 299 citations

    5

    h-index

  4. 3

    h-index

  5. The Astrophysical Journal Letters

    1 publications · 729 citations

    1

    h-index

1–5