Debris Disks

Debris Disk is a circumstellar disk composed predominantly of dust and planetesimals produced by collisions and evaporation of larger bodies, distinguished from protoplanetary disks by its lack of significant gas content and its persistence around mature stars, indicating a later stage in planetary system evolution.

861

Publications

57K

Citations

2K

Authors

630

Institutions

Publications per year

2017–2026

219

Authors

2K

  1. MC
    M. C. Wyatt

    University of Cambridge, United Kingdom

    74 publications · 7.1K citations

    47

    h-index

  2. JA
    J.‐C. Augereau

    Centre National de la Recherche Scientifique, France

    61 publications · 3.7K citations

    41

    h-index

  3. GH
    G. H. Rieke

    University of Arizona, United States

    36 publications · 3.7K citations

    32

    h-index

  4. KY
    K. Y. L. Su

    University of Arizona, United States

    42 publications · 3.7K citations

    32

    h-index

  5. GM
    Grant M. Kennedy

    University of Cambridge, United Kingdom

    46 publications · 2.7K citations

    31

    h-index

1–5 of 2K

Venues

  1. The Astrophysical Journal

    ApJ · 269 publications · 22K citations

    82

    h-index

  2. Astronomy and Astrophysics

    122 publications · 6.7K citations

    51

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    111 publications · 6.4K citations

    46

    h-index

  4. The Astronomical Journal

    AJ · 53 publications · 3.4K citations

    35

    h-index

  5. The Astrophysical Journal Letters

    45 publications · 2.4K citations

    31

    h-index

1–5