Black Hole Accretion with Saturated Magnetic Pressure and Disk Wind
J Huang, H Feng, WM Gu, WB Wu - The Astrophysical Journal, 2023 - iopscience.iop.org
We construct an analytical black hole accretion disk model that incorporates both magnetic
pressure and disk wind, which are found to be important from numerical simulations. A …
pressure and disk wind, which are found to be important from numerical simulations. A …
Do Neutron Star Ultraluminous X-Ray Sources Masquerade as Intermediate-mass Black Holes in Radio and X-Ray?
T Panurach, KC Dage, R Urquhart… - The Astrophysical …, 2024 - iopscience.iop.org
Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-
Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also …
Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also …
Explaining the 'Outliers' Track in Black Hole X-ray Binaries with a BZ-Jet and Inner-Disk Coupling
N Chang, X Liu, FG Xie, L Cui, H Shan - Universe, 2022 - mdpi.com
In this paper, we investigate the black hole (BH) spin contribution to jet power, especially for
the magnetic arrested disk (MAD), where only inner accretion disk luminosity is closely …
the magnetic arrested disk (MAD), where only inner accretion disk luminosity is closely …