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Cited article:

Magnetic Accretion Flow Explains the Hysteresis Q-diagram Seen in Outbursts of Black Hole Low-mass X-Ray Binaries

Jiahui Huang, Hua Feng and Lian Tao
The Astrophysical Journal 985 (2) 217 (2025)
https://doi.org/10.3847/1538-4357/add5e8

Magnetic field transport in geometrically thick discs: multidimensional effects on the field strength and inclination angle

Ryoya Yamamoto and Shinsuke Takasao
Monthly Notices of the Royal Astronomical Society 530 (1) 1218 (2024)
https://doi.org/10.1093/mnras/stae860

A quantitative explanation of the radio – X-ray correlation in black-hole X-ray binaries

Nikolaos D. Kylafis, Pablo Reig and Alexandros Tsouros
Astronomy & Astrophysics 679 A81 (2023)
https://doi.org/10.1051/0004-6361/202346379

The jet emitting disk‐standard accretion disk model applied to the active galactic nuclei ultra violet–X‐ray correlation

S. Barnier, P.‐O. Petrucci, J. Ferreira and G. Marcel
Astronomische Nachrichten 344 (4) (2023)
https://doi.org/10.1002/asna.20230020

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

J. Ferreira, G. Marcel, P.-O. Petrucci, et al.
Astronomy & Astrophysics 660 A66 (2022)
https://doi.org/10.1051/0004-6361/202040165