Journal article
Resolving the nuclear obscuring disk in the Compton-thick Seyfert galaxy NGC 5643 with ALMA
- Abstract:
- We present ALMA Band 612CO(2-1) line and rest-frame 232 GHz continuum observations of the nearby Compton-thick Seyfert galaxy NGC 5643 with angular resolutions 0.″11-0.″26 (9-21 pc). The CO(2-1) integrated line map reveals emission from the nuclear and circumnuclear region with a two-arm nuclear spiral extending ∼10″ on each side. The circumnuclear CO(2-1) kinematics can be fitted with a rotating disk, although there are regions with large residual velocities and/or velocity dispersions. The CO(2-1) line profiles of these regions show two different velocity components. One is ascribed to the circular component and the other to the interaction of the AGN outflow, as traced by the [O iii]λ5007 Åemission, with molecular gas in the disk a few hundred parsecs from the AGN. On nuclear scales, we detected an inclined CO(2-1) disk (diameter 26 pc, FWHM) oriented almost in a north-south direction. The CO(2-1) nuclear kinematics can be fitted with a rotating disk that appears to be tilted with respect to the large-scale disk. There are strong non-circular motions in the central 0.″2-0.″3 with velocities of up to 110 km s-1. In the absence of a nuclear bar, these motions could be explained as radial outflows in the nuclear disk. We estimate a total molecular gas mass for the nuclear disk of M(H2) = 1.1 ×107Moand an H2column density toward the location of the AGN of N(H2) ∼ 5 ×1023cm-2, for a standard CO-to-H2conversion factor. We interpret this nuclear molecular gas disk as the obscuring torus of NGC 5643 as well as the collimating structure of the ionization cone.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 3.1MB, Terms of use)
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- Publisher copy:
- 10.3847/1538-4357/aabe30
Authors
+ Science and Technology Facilities Council
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- Funding agency for:
- Rigopoulou, D
- Grant:
- ST/P000541/1
+ European Research Council
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- Funding agency for:
- Hoenig, S
- Grant:
- ERC-2015-StG-677117
+ Science and Technologies Facilities Council
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- Funding agency for:
- Pereira-Santaella, M
- Gandhi, P
- Rosario, D
- Grant:
- ST/N000919/1
- ST/J003697/2
- ST/N000919/1
- Publisher:
- American Astronomical Society
- Journal:
- Astrophysical Journal More from this journal
- Volume:
- 859
- Issue:
- 2
- Pages:
- 144
- Publication date:
- 2018-06-01
- Acceptance date:
- 2018-04-11
- DOI:
- EISSN:
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1538-4357
- ISSN:
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0004-637X
- Keywords:
- Pubs id:
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pubs:844473
- UUID:
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uuid:8c21cc98-b3ac-4ca2-8af1-f6dc6327c772
- Local pid:
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pubs:844473
- Source identifiers:
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844473
- Deposit date:
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2018-07-12
- ARK identifier:
Terms of use
- Copyright holder:
- © 2018 The American Astronomical Society All rights reserved
- Copyright date:
- 2018
- Notes:
- This is the publisher's version of the article. The final version is available online from American Astronomical Society at: 10.3847/1538-4357/aabe30
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