Inner Disk Holes

Inner Disk Holes is a structural feature in protoplanetary disks characterized by a depleted or absent region of dust and gas in the central few astronomical units, distinguishing it from continuous disk models by indicating potential planet formation or dynamical clearing processes.

74

Publications

7.3K

Citations

353

Authors

187

Institutions

Publications per year

2017–2026

7

Authors

353

  1. NC
    Nuria Calvet

    University of Michigan, United States

    7 publications · 1.1K citations

    7

    h-index

  2. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    7 publications · 821 citations

    7

    h-index

  3. PD
    Paola D’Alessio

    Universidad Nacional Autónoma de México, Mexico

    5 publications · 843 citations

    5

    h-index

  4. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    4 publications · 477 citations

    4

    h-index

  5. BE
    Barbara Ercolano

    Ludwig-Maximilians-Universität München, Germany

    4 publications · 438 citations

    4

    h-index

1–5 of 353

Venues

  1. The Astrophysical Journal

    ApJ · 35 publications · 4.3K citations

    30

    h-index

  2. Astronomy and Astrophysics

    10 publications · 448 citations

    10

    h-index

  3. 4

    h-index

  4. The Astronomical Journal

    AJ · 3 publications · 701 citations

    3

    h-index

  5. The Astrophysical Journal Letters

    3 publications · 182 citations

    3

    h-index

1–5