Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. The IBISCO survey: I. Multiphase discs and winds in the Seyfert galaxy Markarian 509
 

The IBISCO survey: I. Multiphase discs and winds in the Seyfert galaxy Markarian 509

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2021
Author(s)
Zanchettin, M. V.
•
Feruglio, Chiara  
•
BISCHETTI, MANUELA  
•
MALIZIA, ANGELA  
•
Molina, M.  
•
BONGIORNO, ANGELA  
•
DADINA, MAURO  
•
GRUPPIONI, Carlotta  
•
PICONCELLI, Enrico  
•
Tombesi, Francesco  
•
Travascio, A.
•
FIORE, Fabrizio  
DOI
10.1051/0004-6361/202039773
Abstract
We present the analysis of the ALMA CO(2-1) emission line and the underlying 1.2 mm continuum of Mrk509 with spatial resolution of 270 pc. This local Seyfert 1.5 galaxy, optically classified as a spheroid, is known to host a ionised disc, a starburst ring, and ionised gas winds on both nuclear and galactic scales. From CO(2-1) we estimate a molecular gas mass $M_{H_2}=1.7\times 10^9\, \rm M_{\odot}$, located within a disc of size 5.2 kpc, with $M_{dyn}$=(2.0$\pm$1.1) $\times$ $10^{10}\, \rm M_{\odot}$ inclined at $44\pm10$ deg. The molecular gas fraction within the disc is $\mu_{gas}=5\%$. The gas kinematics in the nuclear region within r=700 pc suggests the presence of a warped nuclear disc. Both the presence of a molecular disc with ongoing star-formation in a starburst ring, and the signatures of a minor merger, are in agreement with the scenario where galaxy mergers produce gas destabilization, feeding both star-formation and AGN activity. The spatially-resolved Toomre Q-parameter across the molecular disc is in the range $Q_{gas}=0.5-10$, and shows that the disc is marginally unstable across the starburst ring, and stable at nucleus and in a lopsided ring-like structure located inside of the starburst ring. We find complex molecular gas kinematics and significant kinematics perturbations at two locations, one within 300 pc from the nucleus, and one 1.4 kpc away close to the region with high $Q_{gas}$, that we interpret as molecular winds. The total molecular outflow rate is in the range 6.4-17.0 $\rm M_\odot/yr$. The molecular wind total kinetic energy is consistent with a multiphase momentum-conserving wind driven by the AGN with $\dot{P}_{of}/\dot{P}_{rad}$ in the range 0.06-0.5. The spatial overlap of the inner molecular wind with the ionised wind, and their similar velocity suggest a cooling sequence within a multiphase AGN driven wind.
Funding(s)
2017PH3WAT_001 (Black hole winds and the baryon life cycle of galaxies: the stone-guest at the galaxy evolution supper)  
Volume
655
Start page
A25
Uri
http://hdl.handle.net/20.500.12386/31868
Url
https://www.aanda.org/articles/aa/abs/2021/11/aa39773-20/aa39773-20.html
http://arxiv.org/abs/2107.06756v1
Issn Identifier
0004-6361
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

aa39773-20.pdf

Description
Pdf editoriale
Size

1.78 MB

Format

Unknown

Checksum (MD5)

507c37a7e8a22aceb9204a4d2f534214

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback