Inner Disk Structure

Inner Disk Structure is a theoretical construct in astrophysics that characterizes the physical and dynamical organization of matter in the region of an accretion disk closest to the central compact object, distinguished by relativistic effects, intense radiation fields, and viscosity-driven transport processes.

726

Publications

48.4K

Citations

2.5K

Authors

709

Institutions

Publications per year

2017–2026

174

Authors

2.5K

  1. MB
    M. Benisty

    Centre National de la Recherche Scientifique, France

    22 publications · 1.8K citations

    19

    h-index

  2. FM
    F. Ménard

    Centre National de la Recherche Scientifique, France

    18 publications · 1.4K citations

    17

    h-index

  3. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    19 publications · 1.5K citations

    17

    h-index

  4. JM
    J. M. Mïller

    University of Michigan, United States

    19 publications · 1.5K citations

    17

    h-index

  5. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    17 publications · 1.3K citations

    16

    h-index

1–5 of 2.5K

Venues

  1. The Astrophysical Journal

    ApJ · 303 publications · 22.3K citations

    82

    h-index

  2. Astronomy and Astrophysics

    130 publications · 7.4K citations

    51

    h-index

  3. The Astronomical Journal

    AJ · 45 publications · 3.7K citations

    30

    h-index

  4. The Astrophysical Journal Letters

    32 publications · 2.6K citations

    24

    h-index

  5. Monthly Notices of the Royal Astronomical Society

    35 publications · 1.8K citations

    23

    h-index

1–5