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. Cold molecular outflows in the local Universe and their feedback effect on galaxies
 

Cold molecular outflows in the local Universe and their feedback effect on galaxies

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2019
Author(s)
Fluetsch, A.
•
Maiolino, R.
•
Carniani, S.
•
Marconi, Alessandro  
•
CICONE, CLAUDIA
•
Bourne, M. A.
•
Costa, T.
•
Fabian, A. C.
•
Ishibashi, W.
•
Venturi, G.
DOI
10.1093/mnras/sty3449
Abstract
We study molecular outflows in a sample of 45 local galaxies, both star forming and active galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter/submillimeter Array (ALMA) archive and from the literature. For a subsample, we also compare the molecular outflow with the ionized and neutral atomic phases. We infer an empirical analytical function relating the outflow rate simultaneously to the star formation rate (SFR), LAGN, and galaxy stellar mass; this relation is much tighter than the relations with the individual quantities. The outflow kinetic power shows a larger scatter than in previous, more biased studies, spanning from 0.1 to 5 per cent of LAGN, while the momentum rate ranges from 1 to 30 times LAGN/c, indicating that these outflows can be both energy driven, but with a broad range of coupling efficiencies with the interstellar medium (ISM), and radiation pressure driven. For about 10 per cent of the objects, the outflow energetics significantly exceed the maximum theoretical values; we interpret these as `fossil outflows' resulting from activity of a past strong AGN, which has now faded. We estimate that, in the stellar mass range probed here (> 10^{10} M_{☉}), less than 5 per cent of the outflowing gas escapes the galaxy. The molecular gas depletion time associated with the outflow can be as short as a few million years in powerful AGN; however, the total gas (H2 + H I) depletion times are much longer. Altogether, our findings suggest that even AGN-driven outflows might be relatively ineffective in clearing galaxies of their entire gas content, although they are likely capable of clearing and quenching the central region.
Volume
483
Issue
4
Start page
4586
Uri
http://hdl.handle.net/20.500.12386/30638
Url
https://academic.oup.com/mnras/article/483/4/4586/5253620
Issn Identifier
0035-8711
Ads BibCode
2019MNRAS.483.4586F
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

sty3449.pdf

Description
PDF editoriale
Size

6.29 MB

Format

Adobe PDF

Checksum (MD5)

418dddba553e226e2123b9d781e388e8

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