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Black hole feeding and star formation in NGC 1808

Audibert, A. (author)
Observatoire de Paris,Paris Observatory,Instituto de Astrofísica de Canarias,National Observatory of Athens,Universidad de la Laguna,University of La Laguna
Combes, F. (author)
Collège de France,Observatoire de Paris,Paris Observatory
Burillo, S. G. (author)
Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)
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Hunt, L. K. (author)
Osservatorio Astrofisico di Arcetri,Arcetri Astrophysical Observatory
Eckart, A. (author)
Universität zu Köln,University of Cologne
Aalto, Susanne, 1964 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Casasola, V. (author)
Istituto di Radioastronomia
Boone, F. (author)
Institut de Recherche en Astrophysique et Planétologie (IRAP)
Krips, M. (author)
Institut de Radioastronomie Millimétrique (IRAM)
Viti, Serena (author)
University College London (UCL),Universiteit Leiden (UL),Leiden University (UL)
Muller, Sebastien, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Dasyra, K. M. (author)
National Observatory of Athens,University of Athens
van der Werf, P. (author)
Universiteit Leiden (UL),Leiden University (UL)
Martin, S. (author)
European Southern Observatory Santiago,Atacama Large Millimeter-submillimeter Array (ALMA)
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 (creator_code:org_t)
2021-12-03
2021
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 656
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report on Atacama Large Millimeter Array (ALMA) observations of CO(3-2) emission in the Seyfert2/starburst galaxy NGC1808, at a spatial resolution of 4 pc. Our aim is to investigate the morphology and dynamics of the gas inside the central 0.5 kpc and to probe the nuclear feeding and feedback phenomena. We discovered a nuclear spiral of radius 100 = 45 pc. Within it, we found a decoupled circumnuclear disk or molecular torus of a radius of 0:1300 = 6 pc. The HCN(4-3) and HCO+(4-3) and CS(7-6) dense gas line tracers were simultaneously mapped and detected in the nuclear spiral and they present the same misalignment in the molecular torus. At the nucleus, the HCN/HCO+ and HCN/CS ratios indicate the presence of an active galactic nucleus (AGN). The molecular gas shows regular rotation, within a radius of 400 pc, except for the misaligned disk inside the nuclear spiral arms. The computations of the torques exerted on the gas by the barred stellar potential reveal that the gas within a radius of 100 pc is feeding the nucleus on a timescale of five rotations or on an average timescale of 60 Myr. Some non-circular motions are observed towards the center, corresponding to the nuclear spiral arms. We cannot rule out that small extra kinematic perturbations could be interpreted as a weak outflow attributed to AGN feedback. The molecular outflow detected at 250 pc in the NE direction is likely due to supernovae feedback and it is connected to the kpc-scale superwind.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Keyword

Galaxies: kinematics and dynamics
Galaxies: nuclei
Galaxies: ISM
Galaxies: starburst
Galaxies: individual: NGC 1808
Galaxies: active

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art (subject category)
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