Evidence for Ordered Magnetic Fields in the Quasar Environment

Abstract

At a distance of 20 pc from the purported supermassive black hole powering quasars, temperatures and densities are inferred from optical observations (Osterbrock) to be ~10⁴ K and ~10⁴ cm^-3. Here we present very long baseline interferometry radio observations revealing organized magnetic fields on the parsec scale in the hot plasma surrounding the quasar OQ 172 (1442+101). These magnetic fields rotate the plane of polarization of the radio emission coming from the core and inner jet of the quasar. The derived rotation measure (RM) is 40,000 rad m^-2 in the rest frame of the quasar. Only 10 mas (a projected distance of 68 pc) from the nucleus, the jet absolute values of RM fall to less than 100 rad m^-2.