An Alignment Effect in FR I Radio Galaxies: U-band Polarimetry of the Abell 2597 Cluster Central Galaxy

Details An Alignment Effect in FR I Radio Galaxies: U-band Polarimetry of the Abell 2597 Cluster Central Galaxy An Alignment Effect in FR I Radio Galaxies: U-band Polarimetry of the Abell 2597 Cluster Central Galaxy

1998-10-28

arxiv.org/abs/astro-ph/9810465v1

Astronomy and Astrophysics

Astrophysics

25 pages, 4 figures to appear in the ApJ

Scientific paper

10.1086/307262

We have obtained U-band polarimetry of the spatially extended, blue optical continuum associated with the FR I radio source PKS 2322-122. PKS 2322-122 is located in the Abell 2597 cluster central galaxy. We find a three sigma upper limit to the degree of polarization of the optical continuum of less than 6%. This limit is inconsistent with the blue continuum being primarily scattered light or synchrotron radiation. We can therefore exclude models which attribute the blue continuum to scattered light from an active nucleus that is hidden from direct view. Essentially all of the data pertaining to the blue continuum along the radio source-the ``blue lobes''-indicate that they are regions of recent star formation that may have been induced by an interaction between the radio source and the cool ($<10^4$ K), surrounding gas. We compare the restframe U-band polarized luminosities and 1.4 GHz radio powers of A2597 and A1795 to those for several high redshift radio galaxies exhibiting the alignment effect. We suggest that the fundamental property distinguishing some powerful, high redshift radio galaxies exhibiting the alignment effect, and the lower-power, FR I radio galaxies in cooling flows that exhibit the blue lobe phenomenon, is the strength of the AGN.

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