ASPCS
 
Back to Volume
Paper: Analytical Modeling of Hydromagnetic Jets in AGNs
Volume: 290, Active Galactic Nuclei: from Central Engine to Host Galaxy
Page: 219
Authors: Vlahakis, N.; Köenigl, A.
Abstract: We use exact self-similar solutions of the steady, axisymmetric, relativistic, hydromagnetic equations to study the formation of AGN jets. Our formalism allows us to examine the effects of the thermal, centrifugal, and electromagnetic forces on the flow acceleration and collimation. We apply our analysis to the jet in NGC 6251 and show that the puzzling sub-pc scale acceleration to mildly relativistic speeds recently inferred in this source from VLBI measurements can be attributed to magnetic driving.
Back to Volume