Co-evolution of brightest cluster galaxies and galaxy activity in the host clusters

Mei Ling Huang, Lin Wen Chen

Research output: Contribution to journalArticle

Abstract

We have identified ∼500 relatively relaxed galaxy clusters at low redshift (z < 0.3) from the maxBCG catalog with double radio lobes at the center; about 200 radio counterparts of brightest cluster galaxies (BCGs) of these clusters appear to be wide-angle tailed (WAT) radio sources, indicating ongoing interaction between its host galaxy and the surrounding ICM. Our analysis suggests that the radio power of WAT is positively correlated with the optical luminosities of host BCGs, and increases with redshift; whereas the cluster ellipticity-radio galaxy fraction relation shows no obvious difference between WAT and non-WAT clusters.

Original languageEnglish
Number of pages1
JournalProceedings of the International Astronomical Union
Volume5
Issue numberS267
DOIs
Publication statusPublished - 2009 Aug 1

Fingerprint

coevolution
radio
galaxies
radio galaxies
ellipticity
lobes
catalogs
luminosity
interactions

Keywords

  • Galaxies: clusters: general
  • Galaxies: evolution
  • Radio continuum: galaxies

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Cite this

Co-evolution of brightest cluster galaxies and galaxy activity in the host clusters. / Huang, Mei Ling; Chen, Lin Wen.

In: Proceedings of the International Astronomical Union, Vol. 5, No. S267, 01.08.2009.

Research output: Contribution to journalArticle

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