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Resolving the nuclear obscuring disk in the Compton-thick Seyfert galaxy NGC 5643 with ALMA.

Alonso-Herrero, A. and Pereira-Santaella, M. and García-Burillo, S. and Davies, R. I. and Combes, F. and Asmus, D. and Bunker, A. and Díaz-Santos, T. and Gandhi, P. and González-Martín, O. and Hernán-Caballero, A. and Hicks, E. and Hönig, S. and Labiano, A. and Levenson, N. A. and Packham, C. and Almeida, C. Ramos and Ricci, C. and Rigopoulou, D. and Rosario, D. and Sani, E. and Ward, M. J. (2018) 'Resolving the nuclear obscuring disk in the Compton-thick Seyfert galaxy NGC 5643 with ALMA.', Astrophysical journal., 859 (2). p. 144.

Abstract

We present ALMA Band 6 12CO(2–1) line and rest-frame 232 GHz continuum observations of the nearby Compton-thick Seyfert galaxy NGC 5643 with angular resolutions 0farcs11–0farcs26 (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 Å emission, 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 0farcs2–0farcs3 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 × 107 M ⊙ and an H2 column density toward the location of the AGN of N(H2) ~ 5 × 1023 cm−2, for a standard CO-to-H2 conversion 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.

Item Type:Article
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Status:Peer-reviewed
Publisher Web site:https://doi.org/10.3847/1538-4357/aabe30
Publisher statement:© 2018. The American Astronomical Society. All rights reserved.
Date accepted:11 April 2018
Date deposited:27 June 2018
Date of first online publication:01 June 2018
Date first made open access:27 June 2018

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