Thick Disk Accretion

Thick Disk Accretion is a theoretical model of accretion processes in which the accreting plasma forms a geometrically thick, optically thin, radiation-inefficient structure around a compact object, distinguished from thin disk models by its pressure-supported vertical equilibrium and advective energy transport.

93

Publications

6K

Citations

371

Authors

214

Institutions

Publications per year

2017–2026

9

Authors

371

  1. KM
    Kazuo Makishima

    The University of Tokyo, Japan

    5 publications · 326 citations

    5

    h-index

  2. AK
    Aya Kubota

    The University of Tokyo, Japan

    3 publications · 66 citations

    3

    h-index

  3. PS
    Paula Szkody

    University of Washington, United States

    3 publications · 94 citations

    3

    h-index

  4. SK
    Sandip K. Chakrabarti

    Indian Centre for Space Physics, India

    3 publications · 89 citations

    3

    h-index

  5. TM
    Tsunefumi Mizuno

    Hiroshima University, Japan

    3 publications · 66 citations

    3

    h-index

1–5 of 371

Venues

  1. The Astrophysical Journal

    ApJ · 44 publications · 3K citations

    31

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    12 publications · 1.1K citations

    12

    h-index

  3. 8

    h-index

  4. Astronomy and Astrophysics

    4 publications · 226 citations

    4

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 3 publications · 74 citations

    3

    h-index

1–5