Low X-ray luminosity galaxy clusters - II. Optical properties and morphological content at 0.18 < z < 0.70

NILO CASTELLÓN, JOSÉ LUIS; ALONSO, M. VICTORIA; GARCIA LAMBAS, DIEGO; O'MILL, ANA LAURA; VALOTTO, CARLOS

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

WILEY-BLACKWELL PUBLISHING, INC

Lugar: Londres; Año: 2013 vol. 437 p. 2607 - 2620

0035-8711

This is the second of a series of papers on low X-ray luminosity galaxy clusters, in which we present the r , g and i photometry obtained with Gemini Multi-Object Spectrograph IMAGE at Gemini North and South telescopes for seven systems in the redshift range of 0.18 to 0.70. Optical magnitudes, colours and morphological parameters, namely, concentration index, ellipticity and visual morphological classification, are also given. At lower redshifts, the presence of a well-defined red cluster sequence extending by more than 4 mag showed that these intermediate-mass clusters had reached a relaxed stage. This was confirmed by the small fraction of blue galaxy members observed in the central regions of ∼0.75 Mpc. In contrast, galaxy clusters at higher redshifts had a less important red cluster sequence. We also found that the galaxy radial density profiles in these clusters were well fitted by a single power law. At 0.18