Evidence for Ordered Magnetic Fields in the Quasar Environment
Open Access
- 1 July 1997
- journal article
- research article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 483 (1) , L9-L12
- https://doi.org/10.1086/310725
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.Keywords
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