Disk Flaring

Disk Flaring is a phenomenon in galactic astronomy characterized by the increase in the vertical thickness of the stellar or gaseous components of a galactic disk with increasing radial distance from the galactic center, distinguishing it from uniform disk models by its radial dependence on scale height.

49

Publications

3.2K

Citations

153

Authors

129

Institutions

Publications per year

2017–2026

11

Variants

Galactic Disk Flaring

Authors

153

  1. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    2 publications · 120 citations

    2

    h-index

  2. CP
    C. Pinte

    Centre National de la Recherche Scientifique, France

    2 publications · 168 citations

    2

    h-index

  3. GD
    Gaspard Duchêne

    University of California, Berkeley, United States

    2 publications · 168 citations

    2

    h-index

  4. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    2 publications · 284 citations

    2

    h-index

  5. WT
    W.‐F. Thi

    Centre National de la Recherche Scientifique, France

    2 publications · 95 citations

    2

    h-index

1–5 of 153

Venues

  1. The Astrophysical Journal

    ApJ · 15 publications · 1.7K citations

    14

    h-index

  2. Astronomy and Astrophysics

    10 publications · 430 citations

    10

    h-index

  3. The Astrophysical Journal Supplement Series

    3 publications · 196 citations

    3

    h-index

  4. 3

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 2 publications · 26 citations

    2

    h-index

1–5