Misdirected quasars and evolved stars in distant radio galaxies

Statistics – Computation

Scientific paper

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Galactic Evolution, Interstellar Matter, Optical Polarization, Quasars, Red Shift, Absorption Spectra, Active Galactic Nuclei, Astronomical Models, Astronomical Polarimetry, Computational Astrophysics, Hot Electrons, Line Spectra

Scientific paper

We present the results of spectropolarimetry of radio galaxies with redshift close to 1, complemented by imaging polarimetry. These show: (1) a flat (in flambda) polarized UV continuum, (2) broad polarized Mg II emission line, (3) narrow unpolarized forbidden emission lines, (4) a drop in the polarization of the continuum to the red of 4000 A, (5) a strong absorption feature at 2598 A, and (6) perpendicularity between the E vector of polarization, as measured with imaging polarimetry, and the optical/radio axis. these data provide evidence that distant radio galaxies harbor a quasar which is hidden from direct view but seen by scattering from the interstellar medium in the galaxy. Hot electrons cannot be the dominant scattering agent because of the presence of polarized Mg II lines with a width similar to that observed in quasars. The drop in the continuum polarized to the red of the 4000 A break suggests dilution by a red stellar population. The absorption line at 2598 A is probably due to interstellar Fe II. We discuss a two-component model consisting of a dust scattered quasar and an evolved stellar population, which reproduces simultaneously the polarization measurements and the UV/optical spectra energy distribution. Our results provide strong observational support to the unified model for the most luminous active galactic nuclei and to the idea that the alignment effect in distant radio galaxies is due to scattering, and they add an important tool for te study of the early evolution of galaxies.

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