CLASH-VLT: Environment-driven evolution of galaxies in thez= 0.209 cluster Abell 209

2015/10/19 by M. Annunziatella, A. Mercurio, A. Biviano +19 · 75 citations
Physics and Astronomy · #Abell 2744 #Astronomy and Astrophysical Research #Brightest cluster galaxy #Cluster (spacecraft) #Elliptical galaxy #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy group #Stellar mass #Stellar, planetary, and galactic studies #astro-ph.CO #astro-ph.GA

paper · pdf · doi:10.1051/0004-6361/201527399

published in Astronomy and Astrophysics 585, A160 (EDP Sciences) · 17 pages, 20 figures, A&A in press

arxiv created 2015/10/19 · openalex publication_date 2015/11/18 · arxiv updated 2016/01/20 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. The analysis of galaxy properties, such as stellar masses, colors, sizes and morphologies, and the relations among them and the environment, in which the galaxies reside, can be used to investigate the physical processes driving galaxy evolution.

Citations

• A Wide‐FieldHubble Space TelescopeStudy of the Cluster Cl 0024+16 atz= 0.4. I. Morphological Distributions to 5 Mpc Radius
• Dark Halos: The Flattening of the Density Cusp by Dynamical Friction
• Parametric Recovery of Line‐of‐Sight Velocity Distributions from Absorption‐Line Spectra of Galaxies via Penalized Likelihood
• CANDELS: THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY—THE HUBBLE SPACE TELESCOPE OBSERVATIONS, IMAGING DATA PRODUCTS, AND MOSAICS
• Galactic Stellar and Substellar Initial Mass Function

Cited by

• The stellar mass function of galaxies in Planck-selected clusters at 0.5 < z < 0.7: new constraints on the timescale and location of satellite quenching