Program: GN-2011A-Q-75
Title: | Testing the Galaxy Morphology Evolution in Intermediate Mass Galaxy Clusters |
PI: | Maria Victoria Alonso |
Co-I(s): | Jose Luis Nilo Castellon, Diego Garcia Lambas, Carlos Valotto |
Abstract
The morphology content of galaxy clusters at intermediate redshifts differs significantly from those nearby ones (Dressler et al. 1997, ApJ, 490, 577). Studying clusters at higher redshifts and their connection to present day cluster properties is a subject of debate. Galaxy properties, as morphology, luminosity, mass, age, etc. and intracluster medium are expected to be strongly related to cluster assembly. Massive systems have been widely studied both in the nearby universe and at higher redshifts. Intermediate mass systems were not systematically nor deeply studied. We believe that intermediate mass clusters at intermediate redshifts are very important to understand the galaxy evolution in the herarquical model.
Deep photometric and spectroscopic studies of these intermediate-mass systems at different redshifts would allow us to disentangle the different mechanisms involve in their evolution as ram pressure, galaxy interactions, etc. We propose to perform deep images using GMOS at GEMINI NORTH telescope of 8 intermediate-mass low X-ray galaxy clusters at redshifts between 0.3 < z < 0.7.
Publications using this program's data
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[data]
[ADS] Low X-ray luminosity galaxy clusters - II. Optical properties and morphological content at 0.18 < z < 0.70
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[data]
[ADS] Low X-ray luminosity galaxy clusters - III. Weak lensing mass determination at 0.18 < z < 0.70
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[data]
[ADS] Low X-Ray Luminosity Galaxy Clusters: Main Goals, Sample Selection, Photometric and Spectroscopic Observations