Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Quick Search
My eDoc
Session History
Support Wiki
Direct access to
document ID:

          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 358549.0, MPI für Astronomie / Publikationen_mpia
Resolving the complex structure of the dust torus in the active nucleus of the Circinus galaxy
Authors:Tristram, K. R. W.; Meisenheimer, K.; Jaffe, W.; Schartmann, M.; Rix, H. W.; Leinert, C.; Morel, S.; Wittkowski, M.; Röttgering, H.; Perrin, G.; Lopez, B.; Raban, D.; Cotton, W. D.; Graser, U.; Paresce, F.; Henning, T.
Date of Publication (YYYY-MM-DD):2007
Title of Journal:Astronomy and Astrophysics
Start Page:837
End Page:850
Audience:Not Specified
Abstract / Description:Aims.To test the dust torus model for active galactic nuclei directly, we study the extent and morphology of the nuclear dust distribution in the <ASTROBJ>Circinus galaxy</ASTROBJ> using high resolution interferometric observations in the mid-infrared. Methods: Observations were obtained with the MIDI instrument at the Very Large Telescope Interferometer. The 21 visibility points recorded are dispersed with a spectral resolution of lambda/deltalambda≈30 in the wavelength range from 8 to 13 mum. To interpret the data we used a stepwise approach of modelling with increasing complexity. The final model consists of two black body Gaussian distributions with dust extinction. Results: We find that the dust distribution in the nucleus of Circinus can be explained by two components, a dense and warm disk-like component of 0.4 pc size and a slightly cooler, geometrically thick torus component with a size of 2.0 pc. The disk component is oriented perpendicular to the ionisation cone and outflow and seems to show the silicate feature at 10 mum in emission. It coincides with a nuclear maser disk in orientation and size. From the energy needed to heat the dust, we infer a luminosity of the accretion disk of Lacc = 1010 {L}o, which corresponds to 20% of the Eddington luminosity of the nuclear black hole. We find that the interferometric data are inconsistent with a simple, smooth and axisymmetric dust emission. The irregular behaviour of the visibilities and the shallow decrease of the dust temperature with radius provide strong evidence for a clumpy or filamentary dust structure. We see no evidence for dust reprocessing, as the silicate absorption profile is consistent with that of standard galactic dust. We argue that the collimation of the ionising radiation must originate in the geometrically thick torus component. Conclusions: Based on a great leap forward in the quality and quantity of interferometric data, our findings confirm the presence of a geometrically thick, torus-like dust distribution in the nucleus of Circinus, as required in unified schemes of Seyfert galaxies. Several aspects of our data require that this torus is irregular, or ``clumpy''.
Free Keywords:galaxies: active; galaxies: nuclei; galaxies: Seyfert; galaxies: individual: Seyfert; radiation mechanisms: thermal; techniques: interferometric
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie

The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.