High redshift radio galaxies as tracers of galaxy clusters. XMM-Newton observations

E Belsole*, DM Worrall, MJ Hardcastle

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference Contribution (Conference Proceeding)

Abstract

Distant powerful radio galaxies are useful tracers of galaxy groups and clusters, since through their very existence they point to gaseous atmospheres on scales of at least the radio source diameter. We present new results from XMM-Newton observations of three luminous radio galaxies, where evidence for both radiorelated and cluster mission is seen.

Original languageEnglish
Title of host publicationMULTIWAVELENGTH COSMOLOGY
EditorsM Pilonis
Place of PublicationDORDRECHT
PublisherSpringer
Pages145-148
Number of pages4
ISBN (Print)1-4020-1971-8
Publication statusPublished - 2004
EventConference on Multiwavelength Cosmology - Mykonos Isl, Greece
Duration: 17 Jun 200320 Jun 2003

Publication series

NameASTROPHYSICS AND SPACE SCIENCE LIBRARY
PublisherSPRINGER

Conference

ConferenceConference on Multiwavelength Cosmology
CountryGreece
Period17/06/0320/06/03

Keywords

  • radio galaxies
  • clusters of galaxies
  • X-ray
  • radio
  • MAGNETIC-FIELD STRENGTHS
  • CHANDRA

Cite this

Belsole, E., Worrall, DM., & Hardcastle, MJ. (2004). High redshift radio galaxies as tracers of galaxy clusters. XMM-Newton observations. In M. Pilonis (Ed.), MULTIWAVELENGTH COSMOLOGY (pp. 145-148). (ASTROPHYSICS AND SPACE SCIENCE LIBRARY). Springer.