Disk Instability Model

The Disk Instability Model is a theoretical framework in astrophysics that explains the episodic outbursts in X-ray binaries through thermal-viscous instabilities in the accretion disk, distinguishing it from steady accretion models by attributing variability to opacity-driven transitions in the disk’s ionization state.

263

Publications

20.1K

Citations

591

Authors

354

Institutions

Publications per year

2017–2026

42

Variants

Dim

Authors

591

  1. JP
    J. P. Lasota

    Centre National de la Recherche Scientifique, France

    14 publications · 896 citations

    14

    h-index

  2. AP
    Alan P. Boss

    Carnegie Institution for Science, United States

    10 publications · 1.6K citations

    10

    h-index

  3. JM
    J. M. Hameury

    Centre National de la Recherche Scientifique, France

    10 publications · 701 citations

    10

    h-index

  4. SM
    Shin Mineshige

    Kyoto University, Japan

    9 publications · 469 citations

    9

    h-index

  5. YO
    Yoji Osaki

    The University of Tokyo, Japan

    8 publications · 781 citations

    8

    h-index

1–5 of 591

Venues

  1. The Astrophysical Journal

    ApJ · 97 publications · 9K citations

    50

    h-index

  2. 32

    h-index

  3. Astronomy and Astrophysics

    37 publications · 2K citations

    25

    h-index

  4. 12

    h-index

  5. The Astrophysical Journal Letters

    9 publications · 369 citations

    9

    h-index

1–5