The detection of a large-scale ionised outflow in the local CON galaxy Zw049.057
Artikel i vetenskaplig tidskrift, 2025
Aims. Current co-evolutionary models of galaxies and their supermassive black holes (SMBHs) almost unanimously predict the existence of a heavily dust-obscured nuclear phase, critical in growing the SMBH and providing feedback to the host galaxy. However, this phase is poorly understood. Compact obscured nuclei (CONs) are relatively common in local (ultra-)luminous infrared galaxies and are the most obscured nuclei known to date, offering the opportunity to study the effects of such a dust-obscured phase on the galaxy. This work presents a case study of the local CON Zw049.057; we study the large-scale features of the galaxy and their connection to the ongoing activity of the central CON. Methods. We present new, targeted MUSE observations of the local CON galaxy Zw049.057, which is known to host multiple outflow features within its central few hundred parsecs. By mapping the kinematics of Hα, we analysed the large-scale features of the galaxy. Results. For the first time, we identify a kiloparsec-scale ionised outflow in Zw049.057, traced by Hα emission. Kinematics reveal the outflow to be blueshifted and orientated to the foreground of the stellar disk. The ionisation of this outflow is consistent with shock-heating, which may be related to the presence of a previously identified radio jet in the galaxy.
Galaxies: evolution
Galaxies: active
Galaxies: starburst
ISM: jets and outflows
Galaxies: interactions
Författare
Clare Wethers
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Susanne Aalto
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Santiago Del Palacio
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Boy Lankhaar
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
G. Privon
National Radio Astronomy Observatory
University of Virginia
University of Florida
F. Stanley
Institut de Radioastronomie Millimétrique (IRAM)
J. S. Gallagher III
University of Wisconsin
Mark Gorski
Northwestern University
Sabine König
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
Gustav Olander
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Mamiko Sato
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
R. J. Beswick
University of Manchester
F. Combes
Observatoire de Paris
Aaron S. Evans
National Radio Astronomy Observatory
University of Virginia
I. García-Bernete
Centro de Astrobiologia (CAB)
C. Henkel
Max-Planck-Gesellschaft
King Abdulaziz University
M. Imanishi
National Astronomical Observatory of Japan
S. T. Linden
University of Arizona
J. G. Mangum
National Radio Astronomy Observatory
Sebastien Muller
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium
Y. Nishimura
University of Tokyo
C. Ricci
Universidad Diego Portales
Beijing University of Technology
D. Rigopoulou
University of Oxford
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 704 A195Exploring the Hidden Dusty Nuclei of Galaxies (HIDDeN)
Europeiska forskningsrådet (ERC) (789410), 2018-10-01 -- 2023-09-30.
Ämneskategorier (SSIF 2025)
Atom- och molekylfysik och optik
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202453013