Disk Heating

Disk Heating is a theoretical construct in galactic dynamics that describes the process by which stellar orbits in a galactic disk increase in random motion and vertical oscillation amplitudes over time due to gravitational interactions with spiral arms, molecular clouds, or mergers, leading to disk thickening.

205

Publications

18.1K

Citations

430

Authors

265

Institutions

Publications per year

2017–2026

30

Authors

430

  1. CE
    C. E. Jones

    Western University, Canada

    4 publications · 166 citations

    4

    h-index

  2. DN
    D. N. C. Lin

    University of California, Santa Cruz, United States

    4 publications · 429 citations

    4

    h-index

  3. AC
    Alice C. Quillen

    University of Rochester, United States

    4 publications · 459 citations

    4

    h-index

  4. SM
    S. Michael Fall

    Space Telescope Science Institute, United States

    3 publications · 126 citations

    3

    h-index

  5. RH
    R. H. Durisen

    Indiana University Bloomington, United States

    3 publications · 196 citations

    3

    h-index

1–5 of 430

Venues

  1. The Astrophysical Journal

    ApJ · 63 publications · 9K citations

    42

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    42 publications · 3.4K citations

    31

    h-index

  3. Astronomy and Astrophysics

    21 publications · 858 citations

    17

    h-index

  4. The Astronomical Journal

    AJ · 7 publications · 440 citations

    7

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 190 citations

    4

    h-index

1–5