On the Disappearance of a Cold Molecular Torus around the Low-luminosity Active Galactic Nucleus of NGC 1097
Artikel i vetenskaplig tidskrift, 2017
We used the Atacama Large Millimeter/Submillimeter Array to map the CO(3-2) and the underlying continuum emissions around the type-1low-luminosity active galactic nucleus (LLAGN; bolometric luminosity less than or similar to 10(42) erg. s(-1)) of NGC 1097 at similar to 10 pc resolution. These observations revealed a detailed cold gas distribution within a similar to 100 pc of this LLAGN. In contrast to the luminous Seyfert galaxy NGC 1068, where a similar to 7 pc cold molecular torus was recently revealed, a distinctively dense and compact torus is missing in our CO(3-2) integrated intensity map of NGC 1097. Based on the CO(3-2) flux, the gas mass of the torus of NGC 1097 would be a factor of greater than or similar to 2-3 less than that found for NGC 1068 by using the same CO-to-H-2 conversion factor, which implies less active nuclear star formation and/or inflows in NGC 1097. Our dynamical modeling of the CO(3-2) velocity field implies that the cold molecular gas is concentrated in a thin layer as compared to the hot gas traced by the 2.12 mu m H-2 emission in and around the torus. Furthermore, we suggest that NGC 1097 hosts a geometrically thinner torus than NGC 1068. Although the physical origin of the torus thickness remains unclear, our observations support a theoretical prediction that geometrically thick tori with high opacity will become deficient as AGNs evolve from luminous Seyferts to LLAGNs.
galaxies: ISM
galaxies: active
galaxies: individual (NGC 1097)
galaxies: Seyfert
Författare
T. Izumi
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
K. Kohno
University of Tokyo
Research Center for the Early Universe
K. Fathi
Valhallav. 67
E. Hatziminaoglou
European Southern Observatory
R. I. Davies
Max Planck Institut fur extraterrestrische Physik
S. Martin
European Southern Observatory Santiago
Atacama Large Millimeter-submillimeter Array
S. Matsushita
Institute of Astrophysics and Astronomy, Academia Sinica Taiwan
E. Schinnerer
Max Planck Institut fur Astronomie
D. Espada
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
Sokendai Graduate University for Advanced Studies
Susanne Aalto
Chalmers, Rymd- och geovetenskap, Onsala rymdobservatorium
K. Onishi
Ehime University
J. L. Turner
University of California, Los Angeles
M. Imanishi
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
Sokendai Graduate University for Advanced Studies
K. Nakanishi
Sokendai Graduate University for Advanced Studies
National Institutes of Natural Sciences - National Astronomical Observatory of Japan
D. S. Meier
New Mexico Institute of Mining and Technology
K. Wada
Kagoshima University
N. Kawakatu
National Institute of Technology
T. Nakajima
Nagoya University
Astrophysical Journal Letters
2041-8205 (ISSN) 2041-8213 (eISSN)
Vol. 845 1 L5-Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Infrastruktur
Onsala rymdobservatorium
DOI
10.3847/2041-8213/aa808f