VLBA Polarimetry of Three Powerful Radio Galaxy Cores

Details VLBA Polarimetry of Three Powerful Radio Galaxy Cores VLBA Polarimetry of Three Powerful Radio Galaxy Cores

2001-05-16

arxiv.org/abs/astro-ph/0105285v1

Astronomy and Astrophysics

Astrophysics

Accepted to ApJ, 19 pages including 5 figures

Scientific paper

10.1086/322355

We present sensitive, high dynamic range, Very Long Baseline Array (VLBA) polarimetric observations of the cores of three powerful radio galaxies: 3C166, 3C236 and 3C390.3. Significant polarization is detected in one source (3C166) allowing us to map out the Faraday Rotation Measure (RM) distribution and projected magnetic field direction. The inner jet of 3C166 is found to have a rest frame RM of -2300 rad/m**2, similar to those found in quasars cores. No polarized flux was detected from the other two sources, but in both counterjets are seen. The counterjet in 3C236 was previously known, but the detection in 3C390.3 is a new discovery. We suggest that the low fractional polarization in radio galaxy cores is the result of Faraday depolarization by ionized gas associated with the accretion disk. The lower polarization of radio galaxy cores compared to quasars is then naturally explained by unified models as a result of the viewing angle.

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