Abell 315: reconciling cluster mass estimates from kinematics, X-ray, and lensing

2017/02/17 by A. Biviano, P. Popesso, J. P. Dietrich +5
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics #Classical mechanics #Cluster (spacecraft) #Computer science #Context (archaeology) #Cosmology #Galaxies: Formation, Evolution, Phenomena #Galaxy #Geography #Kinematics #Physics #Redshift #Scientific Research and Discoveries #Weak gravitational lensing #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201629471

published as A&A 602, A20 (2017) · Accepted for publication in A&A. 12 pages, 11 figures

arxiv created 2017/02/17 · openalex publication_date 2017/02/22 · arxiv updated 2017/05/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Context. Determination of cluster masses is a fundamental tool for cosmology. Comparing mass estimates obtained by different probes allows to understand possible systematic uncertainties.

Citations

• Galaxy systems in the optical and infrared
• The impact of mergers on relaxed X-ray clusters - III. Effects on compact cool cores
• Evolution of the Phase‐Space Density in Dark Matter Halos
• RVSAO 2.0: Digital Redshifts and Radial Velocities
• The structural and scaling properties of nearby galaxy clusters
• The SDSS DR6 luminosity functions of galaxies
• Mass estimation in the outer regions of galaxy clusters
• Optical analysis of the poor clusters Abell 610, Abell 725, and Abell 796, containing diffuse radio sources
• Formation of Galaxy Clusters
• Numerical study of halo concentrations in dark-energy cosmologies
• A Textbook Example of a Bow Shock in the Merging Galaxy Cluster 1E 0657-56
• The Structure of Dark Matter Halos in Dwarf Galaxies