Volume 511, February 2010
|Number of page(s)||17|
|Published online||11 March 2010|
Dust tori in radio galaxies
Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700AV Groningen, The Netherlands e-mail: G.van.der.Wolk@astro.rug.nl
Accepted: 20 November 2009
Aims. We investigate the quasar – radio galaxy unification scenario and detect dust tori within radio galaxies of various types.
Methods. Using VISIR on the VLT, we acquired sub-arcsecond (~) resolution N-band images, at a wavelength of 11.85 μm, of the nuclei of a sample of 27 radio galaxies of four types in the redshift range . The sample consists of 8 edge-darkened, low-power Fanaroff-Riley class I (FR-I) radio galaxies, 6 edge-brightened, class II (FR-II) radio galaxies displaying low-excitation optical emission, 7 FR-IIs displaying high-excitation optical emission, and 6 FR-II broad emission line radio galaxies. Out of the sample of 27 objects, 10 nuclei are detected and several have constraining non-detections at sensitivities of 7 mJy, the limiting flux a point source has when detected with a signal-to-noise ratio of 10 in one hour of source integration.
Results. On the basis of the core spectral energy distributions of this sample we find clear indications that many FR-I and several low-excitation FR-II radio galaxies do not contain warm dust tori. At least percent of the high-excitation FR-IIs and almost all of the broad line radio galaxies exhibit excess infrared emission, which must be attributed to warm dust reradiating accretion activity. The FR-I and low-excitation FR-II galaxies are all of low efficiency, which is calculated as the ratio of bolometric to Eddington luminosity . This suggests that thick tori are absent at low accretion rates and/or low efficiencies. The high-excitation FR-II galaxies are a mixed population with three types of nuclei: 1) low efficiency with dust torus; 2) low efficiency with weakly emitting dust torus; and 3) high efficiency with weak dust torus. We argue that the unification viewing angle range 0–45 degrees of quasars should be increased to ~60 degrees, at least at lower luminosities.
Key words: galaxies: active / galaxies: jets / galaxies: nuclei / infrared: galaxies / radiation mechanisms: non-thermal / radiation mechanisms: thermal
© ESO, 2010
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