The obscured BLR in the radio galaxy 3C 234

Astronomy and Astrophysics – Astronomy

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Radio Galaxies, Astronomical Polarimetry, Active Galactic Nuclei, H Alpha Line, Spectral Line Width, Radio Scattering, Polarization Characteristics, Near Infrared Radiation, Visible Spectrum

Scientific paper

We present spectropolarimetric observations of the radio galaxy 3C 234 at optical and, for the first time, near-IR wavelengths. In agreement with previous observations we detect broad H-alpha in total and polarized flux, consistent with the scenario in which the central active nucleus is hidden from view and observed via scattered radiation. We model the flux and polarization properties at optical and near-IR wavelengths, which result in a point-source, cone-based scattering geometry in the optical and an extended source scattering in the near-IR, with a dichroic view to the emission regions, which becomes important only at the longer wavelengths. From this model we calculate an intrinsic H-alpha luminosity of 4.9 x 10 exp 44 erg/s, and an extinction to the near-IR emission region of 60 mag for A(V). The scattered radiation also undergoes extinction, this time by 1 mag for A(V), assuming a source function of a typical stellar-subtracted Seyfert 1 galaxy. We also require that the scatterers are in bulk radial outflow at approximately 600 km/s to explain an observed increase in the intrinsic polarization of the scattered broad H-alpha line in the red wing, and blueshifted narrowline components in polarized flux.

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