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Resolving the Nuclear Obscuring Disk in the Compton-thick Seyfert Galaxy NGC 5643 with ALMA

Alonso-Herrero, A.; Pereira-Santaella, M.; García-Burillo, S.; Davies, R.I.; Combes, F.; Asmus, D.; Bunker, A.; Díaz-Santos, T.; Gandhi, P.; González-Martín, O.; Hernán-Caballero, A.; Hicks, E.; Hönig, S.; Labiano, A.; Levenson, N.A.; Packham, C.; Almeida, C. Ramos; Ricci, C.; Rigopoulou, D.; Rosario, D.; Sani, E.; Ward, M.J.

Resolving the Nuclear Obscuring Disk in the Compton-thick Seyfert Galaxy NGC 5643 with ALMA Thumbnail


Authors

A. Alonso-Herrero

M. Pereira-Santaella

S. García-Burillo

R.I. Davies

F. Combes

D. Asmus

A. Bunker

T. Díaz-Santos

P. Gandhi

O. González-Martín

A. Hernán-Caballero

E. Hicks

S. Hönig

A. Labiano

N.A. Levenson

C. Packham

C. Ramos Almeida

C. Ricci

D. Rigopoulou

D. Rosario

E. Sani



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.

Citation

Alonso-Herrero, A., Pereira-Santaella, M., García-Burillo, S., Davies, R., Combes, F., Asmus, D., …Ward, M. (2018). Resolving the Nuclear Obscuring Disk in the Compton-thick Seyfert Galaxy NGC 5643 with ALMA. Astrophysical Journal, 859(2), Article 144. https://doi.org/10.3847/1538-4357/aabe30

Journal Article Type Article
Acceptance Date Apr 11, 2018
Online Publication Date Jun 1, 2018
Publication Date Jun 1, 2018
Deposit Date Jun 27, 2018
Publicly Available Date Jun 27, 2018
Journal Astrophysical Journal
Print ISSN 0004-637X
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 859
Issue 2
Article Number 144
DOI https://doi.org/10.3847/1538-4357/aabe30

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Copyright Statement
© 2018. The American Astronomical Society. All rights reserved.







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