Aims.To investigate the possible relationships between dynamical status and other important characteristics of galaxy clusters, we conducted a study of X-ray cluster morphology using a sample of 101 clusters at redshift $z\sim0.05$–1 taken from the Chandra archive. Methods.The X-ray morphology is quantitatively characterized by a series of objectively measured simple statistics of the X-ray surface brightness distribution, which are designed to be robust against variations of image quality caused by various exposure times and various cluster redshifts. Using these measures, we quantitatively investigated the relationships between the cluster X-ray morphology and various other cluster characteristics. Results.We found: (...
(Abridged) We present a morphological analysis of 17 X-ray selected clusters at z~0.25, imaged unifo...
We present a novel quantitative scheme of cluster classification based on the morphological properti...
This thesis studies how the morphologies of a large sample of clusters of galaxies can be used to co...
Aims.To investigate the possible relationships between dynamical status and other important charact...
To investigate the relationships between dynamical status and other important characteristics of gal...
Aims. We quantitatively studied the X-ray cluster morphology, and then investigated the relationship...
We present a morphological study of 35 X-ray luminous galaxy clusters at 0.15 < z < 0.3, selected in...
Using Chandra archival data, we quantify the evolution of cluster morphology with redshift. Clusters...
The classification of galaxy clusters according to their X-ray appearance is a powerful tool to disc...
We present a quantitative study of the X-ray morphology of galaxy clusters, as a function of their d...
Evolution of global morphology of galaxy clusters as seen in the X-rays was measured, using a variet...
Context. In recent years multi-wavelength observations have shown the presence of substructures rela...
Context. In the framework of the hierarchical model the intra-cluster medium properties of galaxy cl...
Open AccessContext. In recent years multi-wavelength observations have shown the presence of substru...
X-ray observations of galaxy clusters reveal a large range of morphologies with various degrees of d...
(Abridged) We present a morphological analysis of 17 X-ray selected clusters at z~0.25, imaged unifo...
We present a novel quantitative scheme of cluster classification based on the morphological properti...
This thesis studies how the morphologies of a large sample of clusters of galaxies can be used to co...
Aims.To investigate the possible relationships between dynamical status and other important charact...
To investigate the relationships between dynamical status and other important characteristics of gal...
Aims. We quantitatively studied the X-ray cluster morphology, and then investigated the relationship...
We present a morphological study of 35 X-ray luminous galaxy clusters at 0.15 < z < 0.3, selected in...
Using Chandra archival data, we quantify the evolution of cluster morphology with redshift. Clusters...
The classification of galaxy clusters according to their X-ray appearance is a powerful tool to disc...
We present a quantitative study of the X-ray morphology of galaxy clusters, as a function of their d...
Evolution of global morphology of galaxy clusters as seen in the X-rays was measured, using a variet...
Context. In recent years multi-wavelength observations have shown the presence of substructures rela...
Context. In the framework of the hierarchical model the intra-cluster medium properties of galaxy cl...
Open AccessContext. In recent years multi-wavelength observations have shown the presence of substru...
X-ray observations of galaxy clusters reveal a large range of morphologies with various degrees of d...
(Abridged) We present a morphological analysis of 17 X-ray selected clusters at z~0.25, imaged unifo...
We present a novel quantitative scheme of cluster classification based on the morphological properti...
This thesis studies how the morphologies of a large sample of clusters of galaxies can be used to co...