EDP Sciences
Free access
Volume 396, Number 3, December IV 2002
Page(s) 773 - 786
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20021455

A&A 396, 773-786 (2002)
DOI: 10.1051/0004-6361:20021455

Cluster of galaxies around seven radio-loud QSOs at $\mathsf 1<z<\mathsf{1.6}$

II. K-band images
S. F. Sánchez1 and J. I. González-Serrano2

1  Astrophysikalisches Institut Potsdam (AIP), An der Sternwarte 16, 14482 Potsdam, Germany
2  Instituto de Física de Cantabria, Universidad de Cantabria-CSIC, Avd. de Los Castros S/N, 35005-Santander, Spain
    e-mail: gserrano@ifca.unican.es

(Received 25 July 2002 / Accepted 19 September 2002 )

We have conducted a NIR study of the environments of seven radio-loud quasars at redshifts 1<z<1.6. In present paper we describe deep K band images obtained for the fields of $\sim6\times6$ arcmin around the quasars with 3 $\sigma$ limiting magnitudes of $K\sim20.5$. These fields were previously studied using deep B and R band images (Sánchez & González-Serrano 1999). Using optical and NIR data together, a significant excess of galaxies has been found whose optical-NIR colours, luminosity, spatial scale, and number of galaxies are compatible with clusters at the redshift of the quasar.

We have selected a sample of cluster candidates analyzing the R-K vs. K diagram. A ~25% of the candidates present red optical-NIR colours and an ultraviolet excess. This population has been also found in clusters around quasars at the same redshifts (Tanaka et al. 2000; Haines et al. 2001). These galaxies seem to follow a mixed evolution: a main passive evolution plus late star formation processes. The quasars do not inhabit the core of the clusters, being found in the outer regions. This result agrees with the hypothesis that the origin/feeding mechanism of the nuclear activity is merging processes. The quasars inhabit the region where a collision is most likely to produce a merger.

Key words: galaxies: clusters: general -- quasars: general -- radio continuum: galaxies

Offprint request: S. F. Sánchez, ssanchez@aip.de

SIMBAD Objects

© ESO 2002