Published 2025-01-01
“…Using a lepto-hadronic emission model based on a shocked ambient medium and a shocked wind region created by an AGN accretion disk wind, we identify two viable scenarios that are consistent with the Fermi-LAT data and multiwavelength observations: a hadronic pp -dominated scenario and a leptonic external-
Compton-dominated scenario. Both of these show that future observations with the Cherenkov Telescope Array and the Southern Wide-field
Gamma-
ray Observatory could detect TeV emission from a disk wind in GRS 1734−292. …”
Get full text
Article