Disk Dispersal

Disk Dispersal is a theoretical construct in astrophysics that describes the process by which circumstellar disks lose mass and dissipate over time due to mechanisms such as photoevaporation, accretion, and planet formation, thereby marking the transition from protoplanetary to debris disk phases.

104

Publications

8.7K

Citations

270

Authors

169

Institutions

Publications per year

2017–2026

37

Authors

270

  1. BE
    Barbara Ercolano

    Ludwig-Maximilians-Universität München, Germany

    10 publications · 819 citations

    10

    h-index

  2. CJ
    C. J. Clarke

    University of Cambridge, United Kingdom

    8 publications · 1.4K citations

    8

    h-index

  3. GR
    Giovanni Rosotti

    Leiden University, Netherlands

    7 publications · 341 citations

    7

    h-index

  4. JE
    James E. Owen

    Imperial College London, United Kingdom

    5 publications · 543 citations

    5

    h-index

  5. AF
    A. Frasca

    Osservatorio Astrofisico di Catania, Italy

    4 publications · 58 citations

    4

    h-index

1–5 of 270

Venues

  1. Monthly Notices of the Royal Astronomical Society

    17 publications · 2.1K citations

    17

    h-index

  2. Astronomy and Astrophysics

    19 publications · 1.2K citations

    16

    h-index

  3. The Astrophysical Journal

    ApJ · 17 publications · 2.3K citations

    15

    h-index

  4. The Astrophysical Journal Letters

    9 publications · 457 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 6 publications · 183 citations

    6

    h-index

1–5