Results 1 to 10 of about 2,402,391 (371)
THE PECULIARITIES IN O-TYPE GALAXY CLUSTERS
We present the results of analysis of 2D distribution of galaxies in galaxy cluster fields. The Catalogue of Galaxy Clusters and Groups PF (Panko & Flin) was used as input observational data set.
E. A. Panko, S. I. Emelyanov
doaj +1 more source
Galactic properties that favour star cluster formation: a statistical view [PDF]
The presence or absence of star clusters in galaxies, and the properties of star cluster populations compared to their host galaxy properties, are important observables for validating models of cluster formation, galaxy formation, and galaxy assembly. In this work, we apply a Bayesian approach to fit two models to data from surveys of young clusters in
arxiv +1 more source
The Stellar Population of Stripped Cluster Spiral NGC 4522: A Local Analog to K+A Galaxies? [PDF]
We present observations of the stripped Virgo Cluster spiral NGC 4522, a clear, nearby example of a galaxy currently undergoing ISM-ICM stripping. Utilizing SparsePak integral field spectroscopy on the WIYN 3.5m telescope and GALEX UV photometry, we ...
Hugh H. Crowl+2 more
core +2 more sources
Galaxy subgroups in galaxy clusters [PDF]
Galaxies which fall into clusters as part of the same infall halo can retain correlations due to their shared origin. N-body simulations are used to study properties of such galaxy subgroups within clusters, including their richnesses and prevalence.
openaire +4 more sources
The shapes of galaxy clusters [PDF]
17 pages, postscript, submitted to ...
Theije, P.A.M. de+2 more
openaire +4 more sources
Witnessing the growth of the nearest galaxy cluster [PDF]
We present results from Suzaku Key Project observations of the Virgo Cluster, the nearest galaxy cluster to us, mapping its X-ray properties along four long `arms' extending beyond the virial radius.
A. Simionescu
semanticscholar +1 more source
LINEAR SUBSTRUCTURES IN GALAXY CLUSTERS
We propose detailed scheme that is describing the morphology of linear substructures in galaxy clusters. Our base morphological scheme di- vides galaxy clusters using numerical criteria according the parameters: concentration to the cluster center, the ...
E. Panko+3 more
doaj +1 more source
Formation of Galaxy Clusters [PDF]
Formation of galaxy clusters corresponds to the collapse of the largest gravitationally bound overdensities in the initial density field and is accompanied by the most energetic phenomena since the Big Bang and by the complex interplay between gravity-induced dynamics of collapse and baryonic processes associated with galaxy formation. Galaxy clusters
Kravtsov A., BORGANI, STEFANO
openaire +5 more sources
Mass Distribution in Galaxy Cluster Cores [PDF]
Many processes within galaxy clusters, such as those believed to govern the onset of thermally unstable cooling and active galactic nucleus feedback, are dependent upon local dynamical timescales. However, accurate mapping of the mass distribution within
M. Hogan+10 more
semanticscholar +1 more source
3D-Matched-Filter Galaxy Cluster Finder I: Selection Functions and CFHTLS Deep Clusters [PDF]
We present an optimised galaxy cluster finder, 3D-Matched-Filter (3D-MF), which utilises galaxy cluster radial profiles, luminosity functions and redshift information to detect galaxy clusters in optical surveys.
Adami+53 more
core +3 more sources