Unveiling Multimessenger Emission from Hidden Cores of Microquasars
This study models multimessenger emission from microquasars using three physical scenarios to explain radio to ultra-high-energy gamma ray data. It shows that TeV photons can come from proton-photon (pγ) or proton-proton (pp) interactions depending on the region. The models successfully reproduce multiwavelength data for Cygnus X-1 and X-3, constraining particle acceleration mechanisms.