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
87th Annual Meeting of the Meteoritical Society 2025: Abstracts
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley +1 more source
Cosmic Structure Traced by Precision Measurements of the X-Ray Brightest Galaxy Clusters in the Sky [PDF]
T. H. Reiprich
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
CCD photometry of Abell clusters. I - Magnitudes and redshifts for 84 brightest cluster galaxies
Donald P. Schneider +2 more
openalex +1 more source
A New Dissociative Galaxy Cluster Merger: RM J150822.0+575515.2
Galaxy cluster mergers that exhibit clear dissociation between their dark matter, intracluster gas, and stellar components are great laboratories for probing dark matter properties.
Rodrigo Stancioli +3 more
doaj +1 more source
Line emission in the brightest cluster galaxies of the NOAO Fundamental Plane and Sloan Digital Sky Surveys [PDF]
Louise O. V. Edwards +3 more
openalex +1 more source
On the prevalence of radio-loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flows [PDF]
P. N. Best +4 more
openalex +1 more source
A High-Caliber View of the Bullet Cluster through JWST Strong and Weak Lensing Analyses
The Bullet Cluster (1E 0657-56) is a key astrophysical laboratory for studying dark matter, galaxy cluster mergers, and shock propagation in extreme environments.
Sangjun Cha +7 more
doaj +1 more source
Conduction and the Star Formation Threshold in Brightest Cluster Galaxies [PDF]
G. Mark Voit +5 more
openalex +1 more source

