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Unveiling Multimessenger Emission from Hidden Cores of Microquasars
Microquasars are radio-emitting X-ray binaries with relativistic jets and are established sources of $\sim 100$~TeV gamma rays, making them promising candidates for cosmic-ray acceleration. Motivated by recent detections of $\sim 100~$TeV photons from Cygnus~X-1 and multi-PeV photons from Cygnus~X-3
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