ALMA resolves the torus of NGC 1068: Continuum and molecular line emission
Artikel i vetenskaplig tidskrift, 2016
We used the Atacama Large Millimeter Array (ALMA) to map the emission of the CO(6-5) molecular line and the 432 mu m continuum emission from the 300 pc sized circumnuclear disk (CND) of the nearby Seyfert 2 galaxy NGC 1068 with a spatial resolution of similar to 4 pc. These observations spatially resolve the CND and, for the first time, image the dust emission, the molecular gas distribution, and the kinematics from a 7-10 pc diameter disk that represents the submillimeter counterpart of the putative torus of NGC 1068. We fitted the nuclear spectral energy distribution of the torus using ALMA and near-and mid-infrared (NIR/MIR) data with CLUMPY torus models. The mass and radius of the best-fit solution for the torus are both consistent with the values derived from the ALMA data alone: M-gas(torus) = (1 +/- 0.3) x 10(5) M-circle dot and R-torus = 3.5 +/- 0.5 pc. The dynamics of the molecular gas in the torus show strong non-circular motions and enhanced turbulence superposed on a surprisingly slow rotation pattern of the disk. By contrast with the nearly edge-on orientation of the H2O megamaser disk, we found evidence suggesting that the molecular torus is less inclined (i = 34 degrees-66 degrees) at larger radii. The lopsided morphology and complex kinematics of the torus could be the signature of the Papaloizou-Pringle instability, long predicted to likely drive the dynamical evolution of active galactic nuclei tori.
galaxies: ISM
galaxies: individual (NGC 1068)
galaxies: nuclei
galaxies: kinematics and dynamics
galaxies: Seyfert
Författare
S. G. Burillo
OAN
F. Combes
College de France
C. R. Almeida
Universidad de la Laguna
Instituto Astrofisico de Canarias
A. Usero
OAN
M. Krips
IRAM Institut de RadioAstronomie Millimetrique
A. Alonso-Herrero
CSIC-INTA - Centro de Astrobiologia (CAB)
Susanne Aalto
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
V. Casasola
Osservatorio Astrofisico Di Arcetri
L. K. Hunt
Osservatorio Astrofisico Di Arcetri
S. Martin
European Southern Observatory Santiago
Atacama Large Millimeter-submillimeter Array
S. Viti
UCL
L. Colina
Universidad Autonoma de Madrid
CSIC-INTA - Centro de Astrobiologia (CAB)
Francesco Costagliola
Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik
A. Eckart
Universitat zu Koln
A. Fuente
OAN
C. Henkel
King Abdul Azizi University
Max Planck Institut fur Radioastronomie
I. Marquez
CSIC - Instituto de Astrofísica de Andalucía (IAA)
R. Neri
IRAM Institut de RadioAstronomie Millimetrique
E. Schinnerer
Max Planck Institut fur Astronomie
L. J. Tacconi
Max Planck Institut fur extraterrestrische Physik
P.P. van der Werf
Leiden Observatory Research Institute
Astrophysical Journal Letters
2041-8205 (ISSN) 2041-8213 (eISSN)
Vol. 823 1 Art. no. L12- L12Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.3847/2041-8205/823/1/l12