LX-{sigma} relation of galaxy clusters : J/MNRAS/389/1074


Authors : Shen S. orcid , Kauffmann G., Linden A.V.D. (hide) , Kauffmann G., Linden A.V.D. et..al

Bibcode : 2008MNRAS.389.1074S (ADS) (Simbad) (Objects) (hide)

CDS Keywords : Clusters, galaxy; X-ray sources; Velocity dispersion
UAT : Galaxy clusters, X-ray sources, Galaxy kinematics

Observation (OC)

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Inserted into VizieR : 20-Nov-2009
Last modification : 07-Jul-2024

Radio-loud active galactic nuclei and the L_X_-{sigma} relation of galaxy groups and clusters. (2008)

Keywords : galaxies clusters: general - galaxies: jets

Abstract:We use the ROSAT All-Sky Survey to study the X-ray properties of a sample of 625 groups and clusters of galaxies selected from the Sloan Digital Sky Survey. We stack clusters with similar velocity dispersions and investigate whether their average X-ray luminosities and surface brightness profiles vary with the radio activity level of their central galaxies. We find that at a given value of {sigma}, clusters with a central radio active galactic nucleus (AGN) have more concentrated X-ray surface brightness profiles, larger central galaxy masses and higher X-ray luminosities than clusters with radio-quiet central galaxies. The enhancement in X-ray luminosity is more than a factor of 2, is detected with better than 6{sigma} significance and ...(more)
Abstract: (hide)
We use the RASS to study the X-ray properties of our sample of groups and clusters. The RASS mapped the sky in the soft X-ray band (0.1-2.4keV) with exposure time varying between 400 and 40000s, depending on direction on the sky. The resolution of the RASS images is 45 arcsec.


                
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