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Detection of HCN, HCO+, and HNC in the Mrk 231 molecular outflow. Dense molecular gas in the AGN wind

Aalto, Susanne, 1964 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Burillo, S. G. (author)
Observatorio Astronómico Nacional (OAN),Spanish National Observatory (OAN)
Muller, Sebastien, 1976 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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Winters, J.M. (author)
Institut de Radioastronomie Millimétrique (IRAM)
van der Werf, P. (author)
Universiteit Leiden (UL),Leiden University (UL)
Henkel, C. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG),King Abdulaziz University
Costagliola, Francesco, 1981 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Neri, R. (author)
Institut de Radioastronomie Millimétrique (IRAM)
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 (creator_code:org_t)
2012-01-06
2012
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 537, s. 44-51
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We obtained high-resolution (1.''55 × 1.''28) observations of HCN, HCO+, HNC 1-0 and HC3N 10-9 of the ultraluminous galaxy (ULIRG) Mrk 231 with the IRAM Plateau de Bure Interferometer.Results: We detect luminous emission from HCN, HCO+ and HNC 1-0 in the QSO ULIRG Mrk 231. All three lines show broad line wings - which are particularly prominent for HCN. Velocities are found to be similar ( ≈ ± 750 km s-1) to those found for CO 1-0. This is the first time bright HCN, HCO+ and HNC emission has been detected in a large-scale galactic outflow. We find that both the blue- and red-shifted line wings are spatially extended by at least 0.''75 (>700 pc) in a north-south direction. The line wings are brighter (relative to the line center intensity) in HCN than in CO 1-0 and line ratios suggest that the molecular outflow consists of dense (n > 104 cm-3) and clumpy gas with a high HCN abundance X(HCN) > 10-8. These properties are consistent with the molecular gas being compressed and fragmented by shocks in the outflow. Alternatively, HCN is instead pumped by mid-IR continuum, but we propose that this effect is not strong for the spatially extended outflowing gas. In addition, we find that the rotation of the main disk, in east-west direction, is also evident in the HCN, HCO+ and HNC line emission. An unexpectedly bright HC3N 10-9 line is detected inside the central 400 pc of Mrk 231. This HC3N emission may emerge from a shielded, dust-enshrouded region within the inner 40-50 pc where the gas is heated to high temperatures (200-300 K) by the AGN.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

radio lines: ISM
ISM: molecules
galaxies: active
quasars: general
galaxies: individual: Mrk 231
galaxies: evolution

Publication and Content Type

art (subject category)
ref (subject category)

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