Microquasars are laboratories for the study of jets of relativistic particles produced by accretion onto a spinning black hole. Microquasars are near enough to allow detailed imaging of spatial features across the multiwavelength spectrum. The recent extension measurement of the spatial morphology of a microquasar, SS 433, to TeV gamma rays¹ localizes the acceleration of electrons at shocks in the jet far from the black hole². V4641 Sagittarii (V4641 Sgr) is a similar binary system with a …