Magnetohydrodynamic Winds Driven by the Line Force from the Standard Thin Disk around Supermassive Black Holes. I. The Case of Weak Magnetic Field
Xiao-Hong Yang,
Kamarjan Ablimit,
Qi-Xiu Li
Abstract:The absorption lines with high blue-shifted velocities are frequently found in the ultraviolet (UV) and X-ray spectra of luminous active galactic nuclei (AGNs). This implies that the high-velocity winds/outflows are common in AGNs. In order to study the formation of high-velocity winds, especially ultra-fast outflows (UFOs), we perform two-dimensional magnetohydrodynamic (MHD) simulations. Initially, a magnetic field is set to be weaker than the gas pressure at disk surface. In our simulations, line force oper… Show more
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