EDP Sciences
Free Access
Volume 426, Number 2, November I 2004
Page(s) 445 - 454
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361:20040336
Published online 11 October 2004

A&A 426, 445-454 (2004)
DOI: 10.1051/0004-6361:20040336

The dynamical state of a thick cloudy torus around an AGN

T. Beckert1 and W. J. Duschl2, 1

1  Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
    e-mail: tbeckert@mpifr-bonn.mpg.de
2  Institut für Theoretische Astrophysik der Universität Heidelberg, Tiergartenstraße 15, 69121 Heidelberg, Germany

(Received 25 February 2004 / Accepted 6 July 2004)

We present stationary models of obscuring dusty tori around active galactic nuclei. Vertical and radial structure are discussed separately based on a dynamical approach to a cloudy accretion flow. The vertical cloud distribution is described by a modified isothermal disk for arbitrary thickness of the torus with a wide funnel along the symmetry axis. The radial accretion flow is a consequence of cloud-cloud collisions. Accretion in the combined gravitational potential of central black hole and stellar cluster generates free energy, which is dissipated in collisions, and maintains the thickness of the torus. We focus on the largest clouds at the tidal shear limit, which will dominate the dynamics and the appearance of torus. Successful obscuration as required by unified schemes of AGN is achieved for large mass accretion rates above the Eddington limit of the central black hole. A complete quantitative treatment for the putative torus in the prototypical Seyfert 2 nucleus of NGC 1068 is given.

Key words: accretion, accretion disks -- black hole physics -- ISM: clouds -- galaxies: active -- galaxies: nuclei -- galaxies: individual: NGC 1068

SIMBAD Objects

© ESO 2004

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.