AustralieFrV1, Main, Exploration, bibRecord, 005B20

Jet and torus orientations in high redshift radio galaxies

Identifieur interne : 005B20 ( Main/Exploration ); précédent : 005B19; suivant : 005B21

Jet and torus orientations in high redshift radio galaxies

Auteurs : G. Drouart [Allemagne, France, Australie] ; C. De Breuck [Allemagne] ; J. Vernet [Allemagne] ; R. A. Laing [Allemagne] ; N. Seymour [Australie] ; D. Stern [États-Unis] ; M. Haas [Allemagne] ; E. A. Pier [États-Unis] ; B. Rocca-Volmerange [France]

Source :

Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2012.

RBID : Pascal:13-0063999

Descripteurs français

Pascal (Inist)
- Jet, Tore, Déplacement vers le rouge, Radiogalaxies, Noyau galactique actif, Transfert radiatif, Modèle spectral, Densité spectrale énergie, Observatoire spatial, Corrélation, Photométrie IR, Dégénérescence, Galaxies actives, Continuum, Galaxies infrarouges, Radiosource cosmique, Noyau galaxies.

English descriptors

KwdEn :
- Active galaxies, Active galaxy nuclei, Continuum, Correlations, Cosmic radio sources, Degeneration, Galaxy nuclei, Infrared galaxies, Infrared photometry, Jets, Radiative transfer, Radio galaxies, Red shift, Spatial observatory, Spectral energy distribution, Spectral model, Tori.

Abstract

We examine the relative orientation of radio jets and dusty tori surrounding the active galactic nucleus (AGN) in powerful radio galaxies at z > 1. The radio core dominance R = P^{20 GHz}_core/P^{500 MHz}_extendedserves as an orientation indicator, measuring the ratio between the anisotropic Doppler-beamed core emission and the isotropic lobe emission. Assuming a fixed cylindrical geometry for the hot, dusty torus, we derive its inclination i by fitting optically-thick radiative transfer models to spectral energy distributions obtained with the Spitzer Space Telescope. We find a highly significant anti-correlation (p < 0.0001) between R and i in our sample of 35 type 2 AGN combined with a sample of 18 z ∼ 1 3CR sources containing both type 1 and 2 AGN. This analysis provides observational evidence both for the Unified scheme of AGN and for the common assumption that radio jets are in general perpendicular to the plane of the torus. The use of inclinations derived from mid-infrared photometry breaks several degeneracies which have been problematic in earlier analyses. We illustrate this by deriving the core Lorentz factor Γ from the R-i anti-correlation, finding Γ ? 1.3.

Affiliations:

Allemagne, Australie, France, États-Unis
Île-de-France
Paris

Links toward previous steps (curation, corpus...)

to stream PascalFrancis, to step Corpus: 000C80
to stream PascalFrancis, to step Curation: 005184
to stream PascalFrancis, to step Checkpoint: 000F86
to stream Main, to step Merge: 005E21
to stream Main, to step Curation: 005B20

Le document en format XML

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<profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Active galaxies</term>
<term>Active galaxy nuclei</term>
<term>Continuum</term>
<term>Correlations</term>
<term>Cosmic radio sources</term>
<term>Degeneration</term>
<term>Galaxy nuclei</term>
<term>Infrared galaxies</term>
<term>Infrared photometry</term>
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<term>Radiative transfer</term>
<term>Radio galaxies</term>
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<term>Spectral energy distribution</term>
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<term>Noyau galactique actif</term>
<term>Transfert radiatif</term>
<term>Modèle spectral</term>
<term>Densité spectrale énergie</term>
<term>Observatoire spatial</term>
<term>Corrélation</term>
<term>Photométrie IR</term>
<term>Dégénérescence</term>
<term>Galaxies actives</term>
<term>Continuum</term>
<term>Galaxies infrarouges</term>
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<front><div type="abstract" xml:lang="en">We examine the relative orientation of radio jets and dusty tori surrounding the active galactic nucleus (AGN) in powerful radio galaxies at z > 1. The radio core dominance R = P<sup>20 GHz</sup>
<sub>core</sub>
/P<sup>500 MHz</sup>
<sub>extended </sub>
serves as an orientation indicator, measuring the ratio between the anisotropic Doppler-beamed core emission and the isotropic lobe emission. Assuming a fixed cylindrical geometry for the hot, dusty torus, we derive its inclination i by fitting optically-thick radiative transfer models to spectral energy distributions obtained with the Spitzer Space Telescope. We find a highly significant anti-correlation (p < 0.0001) between R and i in our sample of 35 type 2 AGN combined with a sample of 18 z ∼ 1 3CR sources containing both type 1 and 2 AGN. This analysis provides observational evidence both for the Unified scheme of AGN and for the common assumption that radio jets are in general perpendicular to the plane of the torus. The use of inclinations derived from mid-infrared photometry breaks several degeneracies which have been problematic in earlier analyses. We illustrate this by deriving the core Lorentz factor Γ from the R-i anti-correlation, finding Γ ? 1.3.</div>
</front>
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	Serveur d'exploration sur les relations entre la France et l'Australie
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Serveur d'exploration sur les relations entre la France et l'Australie

Jet and torus orientations in high redshift radio galaxies

Jet and torus orientations in high redshift radio galaxies

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