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
Fundamental parameters of brightest cluster galaxies
Photometry and spectroscopy of a sample of the brightest cluster galaxies (BCGs) are presented, and the relationships between scale length, surface brightness, velocity dispersion, and line strength are determined and compared with the relations determined for lower luminosity ellipticals (LLEs).
John G. Hoessel, W. R. Oegerle
openaire +2 more sources
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
Revisiting Brightest Cluster Galaxy Evolution with the Las Campanas Distant Cluster Survey [PDF]
Amy E. Nelson+3 more
openalex +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
CCD photometry of Abell clusters. I - Magnitudes and redshifts for 84 brightest cluster galaxies
Donald P. Schneider+2 more
openalex +1 more source
Spatial Distribution of Intracluster Light versus Dark Matter in Horizon Run 5
One intriguing approach for studying the dynamical evolution of galaxy clusters is to compare the spatial distributions among various components such as dark matter, member galaxies, gas, and intracluster light (ICL).
Jaewon Yoo+13 more
doaj +1 more source
The environments of the radio galaxy population in simba. [PDF]
Thomas N, Davé R.
europepmc +1 more source
Feedback and Brightest Cluster Galaxy Formation: ACS Observations of the Radio Galaxy TN J1338−1942 atz= 4.1 [PDF]
A. Zirm+45 more
openalex +1 more source
Augmenting astrophysical scaling relations with machine learning: Application to reducing the Sunyaev-Zeldovich flux-mass scatter. [PDF]
Wadekar D+9 more
europepmc +1 more source