Observing positive and negative AGN feedback
arXiv:1802.10305 · doi:10.1038/s41550-018-0404-5
Abstract
Galaxy-scale outflows powered by actively accreting supermassive black holes are routinely detected, and they have been associated both with suppression and triggering of star formation. Recent observational evidence and simulations are favouring a delayed mechanism that connects outflows and star formation
Authors' version, 3 pages and 1 figure, Comment published in Nature Astronomy (View-only version: http://rdcu.be/HUVf)
References in corpus (5)
- Strangulation as the primary mechanism for shutting down star formation in galaxies
- Star formation in a galactic outflow
- Blowin' in the wind: both `negative' and `positive' feedback in an obscured high-z Quasar
- Ionized gas outflows and global kinematics of low-z luminous star forming galaxies
- Evidence for feedback in action from the molecular gas content in the z~1.6 outflowing QSO XID2028
Cited by in corpus (55)
- AGN outflows and feedback twenty years on
- The MAGNUM survey: different gas properties in the outflowing and disk components in nearby active galaxies with MUSE
- MAGNUM survey: A MUSE-Chandra resolved view on ionized outflows and photoionization in the Seyfert galaxy NGC 1365
- The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies
- AGN Feedback and Star Formation of Quasar Host Galaxies: Insights from the Molecular Gas
- Bubbles and outflows: the novel JWST/NIRSpec view of the z=1.59 obscured quasar XID2028
- Ultra-diffuse galaxies without dark matter
- Quasar Feedback Survey: Multi-phase outflows, turbulence and evidence for feedback caused by low power radio jets inclined into the galaxy disk
- High molecular gas content and star formation rates in local galaxies that host quasars, outflows and jets
- The Quasar Feedback Survey: Discovering hidden Radio-AGN and their connection to the host galaxy ionised gas
- Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. II. Spatially Resolved Mass Outflow Rates for the QSO2 Markarian 34
- Two-Face(s): ionized and neutral gas winds in the local Universe
- Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. III. Results for the Seyfert 2 Galaxies Markarian 3, Markarian 78, and NGC 1068
- SUPER I. Toward an unbiased study of ionized outflows in z~2 active galactic nuclei: survey overview and sample characterization
- MUSE view of Arp220: Kpc-scale multi-phase outflow and evidence for positive feedback
- KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at -
- SUPER IV. CO(J=3-2) properties of active galactic nucleus hosts at cosmic noon revealed by ALMA
- Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
- Spatially resolved evidence of the impact of quasar driven outflows on recent star formation : The case of Mrk 34
- Connecting X-ray nuclear winds with galaxy-scale ionised outflows in two lensed quasars
- Quiescent galaxies at : observations vs. models
- Star formation quenching stages of active and non-active galaxies
- SUPER V. ALMA continuum observations of z~2 AGN and the elusive evidence of outflows influencing star formation
- The impact of ionised outflows from z2.5 quasars is not through instantaneous in-situ quenching: the evidence from ALMA and VLT/SINFONI
- The MURALES survey II. Presentation of MUSE observations of 20 3C low-z radio galaxies and first results
- The molecular gas properties in local Seyfert 2 galaxies
- GA-NIFS: JWST/NIRSpec IFS view of the z~3.5 galaxy GS5001 and its close environment at the core of a large-scale overdensity
- MOKA3D: An innovative approach to 3D gas kinematic modelling. I. Application to AGN ionized outflows
- Blazar nature of high-z radio-loud quasars
- Rejuvenation triggers nuclear activity in nearby galaxies
- An ALMA view of 11 Dusty Star Forming Galaxies at the peak of Cosmic Star Formation History
- The MURALES survey. III. Completing the MUSE observations of 37 3C low-z radio galaxies
- Unveiling the Fast Acceleration of AGN-Driven Winds at Kiloparsec Scales
- Compact Molecular Gas Distribution in Quasar Host Galaxies
- A multi-wavelength study of a massive, active galaxy at : coupling the kinematics of the ionized and molecular gas
- HST emission-line images of nearby 3CR radio galaxies: two photoionization, accretion and feedback modes
- Mildly Suppressed Star Formation in Central Regions of MaNGA Seyfert Galaxies
- A search for ionised gas outflows in an Halpha imaging atlas of nearby LINERs
- SUPER VII. Morphology and kinematics of H emission in AGN host galaxies at Cosmic noon using SINFONI
- Imaging Spectroscopy of Ionized Gaseous Nebulae around Optically Faint AGN at Redshift z ~ 2
- Investigating the impact of quasar-driven outflows on galaxies at redshift 0.3-0.4
- Molecular gas and dust properties in quasar hosts
- Star formation efficiency and AGN feedback in narrow-line Seyfert 1 galaxies with fast X-ray nuclear winds
- The Quasar Feedback Survey: zooming into the origin of radio emission with e-MERLIN
- GA-NIFS: Mapping AGN-driven ionized outflows in the COSMOS field
- Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
- The ubiquity of AGN winds in Seyfert 1 galaxies at low redshift
- Does Feedback from Supermassive Blackhole Co-evolve With Host In Type 2 Quasars?
- The [OIII] profiles of far-infrared active and non-active optically-selected green valley galaxies
- MIRACLE II: Unveiling the multi-phase gas interplay in the circumnuclear region of NGC 1365 via multi-cloud modeling
- SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch
- Establishing the impact of powerful AGN on their host galaxies
- What excites the optical emission in X-ray-selected galaxies?
- Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS
- Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. IV. The Effects of Different Density Estimates on the Ionized Gas Masses and Outflow Rates