Lopsidedness of cluster galaxies in modified gravity
We point out an interesting theoretical prediction for elliptical galaxies residing inside galaxy clusters in the framework of modified Newtonian dynamics (MOND), that could be used to test this paradigm.
A. Knebe+13 more
core +2 more sources
The ESO Distant Cluster Survey (EDisCS) is a photometric and spectroscopic study of the galaxy cluster population at two epochs, z~0.5 and z~0.8, drawn from the Las Campanas Distant Cluster Survey (LCDCS).
Anthony H. Gonzalez+7 more
core +1 more source
Spectroscopic and X-ray Modeling of the Strong Lensing Galaxy Cluster MACS J0138.0-2155
We model the total mass and galactic substructure in the strong lensing galaxy cluster MACS J0138.0-2155 using a combination of Chandra X-ray data, Multi-Unit Spectroscopic Explorer (MUSE) spectroscopy, and Hubble Space Telescope imaging.
Abigail Flowers+4 more
doaj +1 more source
Alignment Effects of Brightest Cluster Galaxies [PDF]
D. G. Lambas+2 more
openalex +1 more source
The transformation of Spirals into S0 galaxies in the cluster environment
We discuss the observational evidences of the morphological transformation of Spirals into S0 galaxies in the cluster environment exploiting two big databases of galaxy clusters: WINGS (0 ...
Mauro eD'onofrio+2 more
doaj +1 more source
The Globular Cluster Luminosity Functions of Brightest Cluster Galaxies [PDF]
John P. Blakeslee
openalex +1 more source
Using Neural Networks to Automate the Identification of Brightest Cluster Galaxies in Large Surveys
Brightest cluster galaxies (BCGs) lie deep within the largest gravitationally bound structures in existence. Though some cluster finding techniques identify the position of the BCG and use it as the cluster center, other techniques may not automatically ...
Patrick Janulewicz+2 more
doaj +1 more source
The K-Band Hubble Diagram for the Brightest Cluster Galaxies: A Test of Galaxy Formation Models [PDF]
Alfonso Aragón‐Salamanca+2 more
openalex +1 more source
A Multiwavelength Approach to Constraining the Merger Properties of ACT-CL J0034.4+0225
ACT-CL J0034.4+0225 is a previously unrecognized merging galaxy cluster at z = 0.38588 ± 0.00068. Our primary evidence is provided by a 21 ks Chandra image that shows two surface brightness peaks separated by ∼49″ (259 kpc) surrounded by an extended ...
Peter Doze+12 more
doaj +1 more source
A Kinematic Search for Bound Populations around Brightest Cluster Members in a Sample of 52 Clusters of Galaxies [PDF]
D. Bottini
openalex +1 more source