Clumpy tori illuminated by the anisotropic radiation of accretion discs in active galactic nuclei

Abstract

In this paper, we try to explain the observed correlation between the covering factor (CF) of hot dust and the properties of active galactic nuclei (AGNs), e.g., the bolometric luminosity ($L_{\mathrm{bol}}$) and black hole mass ($M_{\mathrm{BH}}$). Combining the possible dust distribution in the torus, the angular dependence of the radiation of the accretion disc, and the relation between the critical angle of torus and the Eddington ratio, there are eight possible models investigated in our work. We fit the observed CF with these models to determine the parameters of them. As a result, clumpy torus models can generally explain the observed correlations of tori, while the smooth models fail to produce the required CFs. However, there is still significant scatter even for the best-fitting model, which is the combination of a clumpy torus illuminated by the anisotropic radiation of accretion disc in an AGN. Although some of the observed scatter is due to the uncertainties in measuring $L_{\mathrm{bol}}$ and $M_{\mathrm{BH}}$, other factors are required in more realistic model. The models examined in this paper are not necessary to be the physical model of tori. However, the reasonable assumptions selected during this process should be helpful in constructing physical models of tori.

12 pages, 11 figures, 3 tables. To be published in MNRAS

References in corpus (12)

• AGN Dusty Tori: I. Handling of Clumpy Media
• Dust covering factor, silicate emission and star formation in luminous QSOs
• CAIXA: a Catalogue of AGN In the XMM-Newton Archive I. Spectral analysis
• Black Hole Growth to z = 2 - I: Improved Virial Methods for Measuring M_BH and L/L_Edd
• Smooth and Clumpy Dust Distribution in AGN: a Direct Comparison of two Commonly Explored Infrared Emission Models
• Radiation-driven Fountain and Origin of Torus around Active Galactic Nuclei
• Measuring the Fraction of Obscured Quasars by the Infrared Luminosity of Unobscured Quasars
• IR-derived covering factors for a large sample of quasars from WISE-UKIDSS-SDSS
• Time-resolved infrared emission from radiation-driven central obscuring structures in Active Galactic Nuclei
• AGN obscuration from winds: from dusty infrared-driven to warm and X-ray photoionized
• The Covering Factor of Warm Dust in Quasars: View from WISE All-Sky Data Release
• Single-Epoch Black Hole Mass Estimators For Broad-Line Active Galactic Nuclei: Recalibrating Hbeta with A New Approach

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• A unifying evolutionary framework for infrared-selected obscured and unobscured quasar host haloes
• The Impact of the Dusty Torus on Obscured Quasar Halo Mass Measurements