The influence of AGN feedback on galaxy cluster observables

H. Y. Yang, P. M. Ricker, P. M. Sutter

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Galaxy clusters are valuable cosmological probes. However, cluster mass estimates rely on observable quantities that are affected by complicated baryonic physics in the intracluster medium (ICM), including feedback from active galactic nuclei (AGN). Cosmological simulations have started to include AGN feedback using subgrid models. In order to make robust predictions, the systematics of different implementations and parametrizations need to be understood. We have developed an AGN subgrid model in FLASH that supports a few different black hole accretion models and feedback models. We use this model to study the effect of AGN on X-ray cluster observables and its dependence on model variations.

Original languageEnglish (US)
Title of host publicationMonster's Fiery Breath
Subtitle of host publicationFeedback in Galaxies, Groups, and Clusters - Proceedings of the International Conference
Pages350-353
Number of pages4
DOIs
StatePublished - 2009
Externally publishedYes
EventInternational Conference on Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters - Madison, WI, United States
Duration: Jun 1 2009Jun 5 2009

Publication series

NameAIP Conference Proceedings
Volume1201
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

OtherInternational Conference on Monster's Fiery Breath: Feedback in Galaxies, Groups, and Clusters
CountryUnited States
CityMadison, WI
Period6/1/096/5/09

Keywords

  • Active galactic nuclei
  • Cooling flows
  • Galaxies: clusters
  • Hydrodynamics
  • Methods: numerical

ASJC Scopus subject areas

  • Ecology, Evolution, Behavior and Systematics
  • Ecology
  • Plant Science
  • Physics and Astronomy(all)
  • Nature and Landscape Conservation

Fingerprint Dive into the research topics of 'The influence of AGN feedback on galaxy cluster observables'. Together they form a unique fingerprint.

Cite this