Abstract: BHJet models steady-state SEDs of jets launched from accreting black holes. This semi-analytical, multi-zone jet model is applicable across the entire black hole mass scale, from black hole X-ray binaries (both low and high mass) to active galactic nuclei of any class (from low-luminosity AGN to flat spectrum radio quasars). It is designed to be more comparable than other codes to GRMHD simulations and/or RMHD semi-analytical solutions.
Credit: Lucchini, M.; Ceccobello, C.; Markoff, S.; Kini, Y.; Chhotray, A.; Connors, R. M. T.; Crumley, P.; Falcke, H.; Kantzas, D.; Maitra, D.
Preferred citation method: Please see citation information here: https://github.com/matteolucchini1/BHJet#citing-bhjet