The central dusty torus in the active nucleus of NGC 1068

Abstract : Active galactic nuclei (AGNs) display many energetic phenomena—broad emission lines, X-rays, relativistic jets, radio lobes—originating from matter falling onto a supermassive black hole. It is widely accepted that orientation effects play a major role in explaining the observational appearance of AGNs. Seen from certain directions, circum-nuclear dust clouds would block our view of the central powerhouse1,2. Indirect evidence suggests that the dust clouds form a parsec-sized torus-shaped distribution. This explanation, however, remains unproved, as even the largest telescopes have not been able to resolve the dust structures. Here we report interferometric mid-infrared observations that spatially resolve these structures in the galaxy NGC 1068. The observations reveal warm (320 K) dust in a structure 2.1 parsec thick and 3.4 parsec in diameter, surrounding a smaller hot structure. As such a configuration of dust clouds would collapse in a time much shorter than the active phase of the AGN3, this observation requires a continual input of kinetic energy to the cloud system from a source coexistent with the AGN.
Complete list of metadatas

https://hal.archives-ouvertes.fr/hal-00002348
Contributor : Didier Fraix-Burnet <>
Submitted on : Wednesday, July 28, 2004 - 11:26:52 AM
Last modification on : Wednesday, July 3, 2019 - 10:56:16 AM

Links full text

Identifiers

Collections

OBSPM | INSU | CNRS | LAOG | GEMINI | OSUG | UGA | PSL

Citation

W. Jaffe, K. Meisenheimer, H. J. A. Roettgering, Ch. Leinert, A. Richichi, et al.. The central dusty torus in the active nucleus of NGC 1068. Nature, Nature Publishing Group, 2004, 429, pp.47-49. ⟨10.1038/nature02531⟩. ⟨hal-00002348⟩

Share

Metrics

Record views

305