2016/02/29 by C. Maier, U. Kuchner, B. L. Ziegler +9 · 34 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Brightest cluster galaxy #Cluster (spacecraft) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy group #Galaxy groups and clusters #Quenching (fluorescence) #Universe #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201628223
published in Astronomy and Astrophysics 590, A108 (EDP Sciences) · Version better matched to the published version, including table with observed and derived quantities for the 76 cluster galaxies
openalex publication_date 2016/04/05 · openalex created_date 2016/06/24 · arxiv created 2017/05/05 · arxiv updated 2017/05/08 · openalex updated_date 2026/08/05
Aims. Environmental effects gain importance as large scale structures in the Universe develop with time and have become the dominant mechanism for quenching galaxies of intermediate and low stellar masses at lower redshifts. Therefore, clusters of galaxies at z< 0.5 are the sites where environmental effects are expected to be more pronounced and more easily observed with present-day large telescopes.