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arXiv · astro-ph/9909215

Polarimetry and Unification of Low-Redshift Radio Galaxies

M. H. Cohen·P. M. Ogle·H. D. Tran·R. W. Goodrich·J. S. Miller
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Abstract

We have made high-quality measurements of the polarization spectra of 13 FR II radio galaxies and taken polarization images for 11 of these with the Keck telescopes. Seven of the eight narrow-line radio galaxies (NLRG) are polarized, and six of the seven show prominent broad Balmer lines in polarized light. The broad lines are also weakly visible in total flux. Some of the NLRG show bipolar regions with roughly circumferential polarization vectors, revealing a large reflection nebula illuminated by a central source. Our observations powerfully support the hidden quasar hypothesis for some NLRG. Classification as NLRG, broad-line radio galaxy (BLRG), or quasar therefore depends on orientation. However, not all objects fit into this unification scheme. Our sample is biased towards objects known in advance to be polarized, but the combination of our results with those of Hill, Goodrich and DePoy (1996) show that at least 6 out of a complete, volume and flux-limited sample of 9 FR II NLRG have broad lines, seen either in polarization or P_alpha.

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M. H. Cohen, P. M. Ogle, H. D. Tran, R. W. Goodrich, J. S. Miller. 1999-09-13. Polarimetry and Unification of Low-Redshift Radio Galaxies. https://doi.org/10.1086/301074

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