Extreme Scale Height Variations and Nozzle Shocks in Warped Disks

Accretion disks around both stellar-mass and supermassive black holes (BHs) are likely often warped. Whenever a disk is warped, its scale height varies with azimuth. Sufficiently strong warps cause extreme compressions of the scale height, which fluid parcels “bounce” off of twice per orbit to high...

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Bibliographic Details
Main Authors: Nicholas Kaaz, Yoram Lithwick, Matthew Liska, Alexander Tchekhovskoy
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ad9a85
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