Disk Temperature Structure

Disk Temperature Structure is a theoretical construct that specifies the radial and vertical distribution of thermal energy within a circumstellar disk, distinguishing it from other disk properties by characterizing the spatial variation of temperature as a function of distance from the central star and height above the midplane.

313

Publications

17.6K

Citations

789

Authors

392

Institutions

Publications per year

2017–2026

72

Authors

789

  1. SM
    Sean M. Andrews

    Center for Astrophysics Harvard & Smithsonian, United States

    12 publications · 1.1K citations

    12

    h-index

  2. DJ
    David J. Wilner

    Center for Astrophysics Harvard & Smithsonian, United States

    11 publications · 1.1K citations

    11

    h-index

  3. EF
    E. F. van Dishoeck

    Leiden University, Netherlands

    11 publications · 707 citations

    11

    h-index

  4. IK
    I. Kamp

    Centre National de la Recherche Scientifique, France

    10 publications · 667 citations

    10

    h-index

  5. FM
    F. Ménard

    Centre National de la Recherche Scientifique, France

    8 publications · 529 citations

    8

    h-index

1–5 of 789

Venues

  1. The Astrophysical Journal

    ApJ · 116 publications · 8.3K citations

    49

    h-index

  2. Astronomy and Astrophysics

    39 publications · 2.4K citations

    28

    h-index

  3. 13

    h-index

  4. 13

    h-index

  5. The Astrophysical Journal Letters

    12 publications · 1.2K citations

    12

    h-index

1–5