Reality and Myths of AGN Feedback
arXiv:1802.10304 · doi:10.1038/s41550-018-0407-2
Abstract
Feedback from active galactic nuclei (AGN) remains controversial despite its wide acceptance as necessary to regulate massive galaxy growth. A dedicated workshop was held on 16-20 October 2017 at the Lorentz Center in Leiden to distinguish between the reality and myths of AGN feedback from the observational side. Here, we summarize briefly all the sessions and outcome of the stimulating workshop. More details on the outcome of the discussions are provided in a series of articles.
arXiv commentAuthor's version of Nature Astronomy Meeting Report. View-only version of full text publicly available at this link: http://rdcu.be/HUTV
References in corpus (5)
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
- AGN outflows and feedback twenty years on
- The largely unconstrained multiphase nature of outflows in AGN host galaxies
- Questions and challenges of what powers galactic outflows in active galactic nuclei
Cited by in corpus (13)
- QSO MUSEUM I: A sample of 61 extended Ly-emission nebulae surrounding quasars
- Major mergers are not the dominant trigger for high-accretion AGNs at z = 2
- The Close AGN Reference Survey (CARS): IFU survey data and the BH mass dependence of long-term AGN variability
- A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2
- Star formation quenching stages of active and non-active galaxies
- Simba: The average properties of the circumgalactic medium of quasars are determined primarily by stellar feedback
- SDSS J211852.96-073227.5: The first non-local, interacting, late-type intermediate Seyfert galaxy with relativistic jets
- Mass and Environment as Drivers of Galaxy Evolution. IV. On the Quenching of Massive Central Disk Galaxies in The Local Universe
- Detecting the halo heating from AGN feedback with ALMA
- Investigating the link between inner gravitational potential and star-formation quenching in CALIFA galaxies
- The Close AGN Reference Survey (CARS): No evidence of galaxy-scale hot outflows in two nearby AGN
- The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution
- Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect