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ALMA OBSERVATIONS OF THE SUBMILLIMETER DENSE MOLECULAR GAS TRACERS IN THE LUMINOUS TYPE-1 ACTIVE NUCLEUS OF NGC 7469

Izumi, T. (author)
University of Tokyo, Japan
Kohno, K. (author)
University of Tokyo, Japan
Aalto, Susanne, 1964 (author)
Chalmers tekniska högskola,Chalmers University of Technology
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Doi, A. (author)
Espada, D. (author)
The Graduate University for Advanced Studies (SOKENDAI),National Astronomical Observatory of Japan,Atacama Large Millimeter-submillimeter Array (ALMA)
Fathi, K. (author)
Harada, N. (author)
Academia Sinica Taiwan
Hatsukade, B. (author)
National Astronomical Observatory of Japan
Hattori, T. (author)
National Astronomical Observatory of Japan
Hsieh, P. Y. (author)
Academia Sinica Taiwan,National Central University
Ikarashi, S. (author)
University of Tokyo, Japan,European Southern Observatory (ESO)
Imanishi, M. (author)
National Astronomical Observatory of Japan,The Graduate University for Advanced Studies (SOKENDAI)
Iono, D. (author)
The Graduate University for Advanced Studies (SOKENDAI),National Astronomical Observatory of Japan
Ishizuki, S. (author)
National Astronomical Observatory of Japan
Krips, M. (author)
Institut de Radioastronomie Millimétrique (IRAM)
Martin, S. (author)
Institut de Radioastronomie Millimétrique (IRAM)
Matsushita, S. (author)
Academia Sinica Taiwan
Meier, D. S. (author)
New Mexico Institute of Mining and Technology
Nagai, H. (author)
National Astronomical Observatory of Japan
Nakai, N. (author)
University of Tsukuba
Nakajima, T. (author)
Nagoya University
Nakanishi, K. (author)
National Astronomical Observatory of Japan,Atacama Large Millimeter-submillimeter Array (ALMA),The Graduate University for Advanced Studies (SOKENDAI)
Nomura, H. (author)
Tokyo Institute of Technology
Regan, M. W. (author)
Space Telescope Science Institute (STScI)
Schinnerer, E. (author)
Max Planck Gesellschaft zur Förderung der Wissenschaften e.V. (MPG),Max Planck Society for the Advancement of Science (MPG)
Sheth, K. (author)
National Radio Astronomy Observatory
Takano, S. (author)
Nihon University
Tamura, Y. (author)
University of Tokyo, Japan
Terashima, Y. (author)
Ehime University
Tosaki, T. (author)
Joetsu University of Education
Turner, J. L. (author)
University of California
Umehata, H. (author)
University of Tokyo, Japan
Wiklind, Tommy, 1957 (author)
Atacama Large Millimeter-submillimeter Array (ALMA)
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 (creator_code:org_t)
2015-09-16
2015
English.
In: Astrophysical Journal. - : American Astronomical Society. - 1538-4357 .- 0004-637X. ; 811:1, s. Article Number: 39-
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We present Atacama Large Millimeter/submillimeter Array (ALMA) Cycle 1 observations of the central kiloparsec region of the luminous type. 1 Seyfert galaxy NGC 7469 with unprecedented high resolution (0.'' 5x0.'' 4 = 165 x 132 pc) at submillimeter wavelengths. Utilizing the wide. bandwidth of ALMA, we simultaneously obtained HCN(4-3), HCO+(4-3), CS(7-6), and partially CO(3-2) line maps, as well as the 860 mu m continuum. The region consists of the central similar to 1 '' component and the surrounding starburst ring with a radius of similar to 1.'' 5-2.'' 5. Several structures connect these components. Except for CO(3-2), these dense gas tracers are significantly concentrated toward the central similar to 1 '', suggesting their suitability to probe the nuclear regions of galaxies. Their spatial distribution resembles well those of centimeter and mid-infrared continuum emissions, but it is anticorrelated with the optical one, indicating the existence of dust-obscured star formation. The integrated intensity ratios of HCN(4-3)/HCO+(4-3) and HCN(4-3)/CS(7-6) are higher at the active galactic nucleus (AGN) position than at the starburst ring, which is consistent with our previous findings (submillimeter-HCN enhancement). However, the HCN(4-3)/HCO+(4-3) ratio at the AGN position of NGC 7469 (1.11 +/- 0.06) is almost half of the corresponding value of the low-luminosity type. 1 Seyfert galaxy NGC 1097 (2.0 +/- 0.2), despite the more than two orders of magnitude higher X-ray luminosity of NGC 7469. But the ratio is comparable to that of the close vicinity of the AGN of NGC 1068 (similar to 1.5). Based on these results, we speculate that some heating mechanisms other than X-ray (e.g., mechanical heating due to an AGN jet) can contribute significantly for shaping the chemical composition in NGC 1097.

Subject headings

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

Keyword

agn-driven outflow
1995
galaxies: active
galactic
x-ray
star-formation
supermassive black-hole
nearby
photon-dominated regions
galaxies: ISM
seyfert-galaxies
cloverleaf quasar
infrared galaxies
Astronomy & Astrophysics
broad-line region
astrophysical journal
nuclei
galaxies: individual (NGC 7469)
p129
v444
nzel r
ISM: molecules

Publication and Content Type

art (subject category)
ref (subject category)

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