Puffy Accretion Disks: Sub-Eddington, Optically Thick, and Stable-Reference-Cited by-同舟云学术

Puffy Accretion Disks: Sub-Eddington, Optically Thick, and Stable

Published:2019-10-15 Issue:2 Volume:884 Page:L37
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Lančová Debora^ORCID,Abarca David,Kluźniak Włodek,Wielgus Maciek^ORCID,Sa̧dowski Aleksander,Narayan Ramesh,Schee Jan,Török Gabriel^ORCID,Abramowicz Marek

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/ab48f5/pdf

Reference51 articles.

1. Slim accretion disks

2. Instability, turbulence, and enhanced transport in accretion disks

3. Magnetically elevated accretion discs in active galactic nuclei: broad emission-line regions and associated star formation

4. Oscillation modes of relativistic slender tori

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