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Nuclear molecular outflow in the Seyfert galaxy NGC 3227

Abstract:

ALMA observations have revealed nuclear dusty molecular disks or tori with characteristic sizes 15−40 pc in the few Seyferts and low -luminosity AGN that have been studied so far. These structures are generally decoupled both morphologically and kinematically from the host galaxy disk. We present ALMA observations of the CO(2–1) and CO(3–2) molecular gas transitions and associated (sub-) millimeter continua of the nearby Seyfert 1.5 galaxy NGC 3227 with angular resolutions 0.085 − 0.21″ (7–15...

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Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1051/0004-6361/201935431

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Sub department:
Astrophysics
Role:
Author
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Publisher:
EDP Sciences Publisher's website
Journal:
Astronomy and Astrophysics Journal website
Volume:
628
Article number:
A65
Publication date:
2019-08-08
Acceptance date:
2019-06-12
DOI:
EISSN:
1432-0746
ISSN:
0004-6361
Source identifiers:
1022235
Keywords:
Pubs id:
pubs:1022235
UUID:
uuid:a7aa295d-5e0d-4faa-9c91-ebb824bbb90e
Local pid:
pubs:1022235
Deposit date:
2019-06-25

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