Are low-frequency quasi-periodic oscillations in accretion flows the disk response to jet instability?

Are low-frequency quasi-periodic oscillations in accretion flows the disk response to jet instability?

Low-frequency quasi-periodic oscillations, or LFQPOs, are ubiquitous in black hole X-ray binaries and provide strong constraints on the accretion-ejection processes. Although several models have been proposed, none has been proven to reproduce all observational constraints, and no consensus has emer...

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Bibliographic Details
Main Authors: Belmont, R. (Author), Clavel, M. (Author), Corbel, S. (Author), Coriat, M. (Author), Ferreira, J. (Author), Henri, G. (Author), Malzac, J. (Author), Marcel, G. (Author), Petrucci, P.-O (Author), Rodriguez, J. (Author)
Format: Article
Language:English
Published: EDP Sciences 2022
Subjects:
Accretion discs
Accretion, accretion disks
Accretion: accretion disks
Black holes
Galaxies
Galaxies active
Galaxies: active
Gravitation
ISM jets and outflows
ISM: jets and outflows
Jet instability
Lower frequencies
Magnetohydrodynamic
Magnetohydrodynamics
Magnetohydrodynamics (MHD)
Oscillators (mechanical)
Quasiperiodic oscillations
Stability
Stars
X-rays: binaries
X-rays: Binaries
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