Disk Inclination Effects

Disk Inclination Effects is a theoretical construct in astrophysics that characterizes the observational and physical manifestations arising from the angular orientation of a circumstellar disk relative to the line of sight, distinguishing it by its influence on the interpretation of disk morphology, kinematics, and emission profiles in astronomical measurements.

241

Publications

15.5K

Citations

807

Authors

373

Institutions

Publications per year

2017–2026

60

Authors

807

  1. CP
    C. Pinte

    Centre National de la Recherche Scientifique, France

    8 publications · 538 citations

    9

    h-index

  2. AM
    A. Marconi

    Arcetri Astrophysical Observatory, Italy

    6 publications · 352 citations

    6

    h-index

  3. GM
    Grant M. Kennedy

    University of Cambridge, United Kingdom

    5 publications · 292 citations

    5

    h-index

  4. MC
    M. C. Wyatt

    University of Cambridge, United Kingdom

    4 publications · 240 citations

    5

    h-index

  5. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    4 publications · 332 citations

    4

    h-index

1–5 of 807

Venues

  1. The Astrophysical Journal

    ApJ · 80 publications · 6K citations

    43

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    46 publications · 2.7K citations

    29

    h-index

  3. Astronomy and Astrophysics

    27 publications · 1.8K citations

    21

    h-index

  4. The Astrophysical Journal Letters

    8 publications · 1.5K citations

    9

    h-index

  5. The Astronomical Journal

    AJ · 8 publications · 554 citations

    8

    h-index

1–5