2014/01/31 by P. Saracco, A. Casati, A. Gargiulo +12 · 25 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Brightest cluster galaxy #Cluster (spacecraft) #Context (archaeology) #Elliptical galaxy #Fundamental plane (elliptical galaxies) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy groups and clusters #Geography #Geometry #Lenticular galaxy #Physics #Scaling #Stellar, planetary, and galactic studies #Surface brightness #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201423495
published in Astronomy and Astrophysics 567, A94 (EDP Sciences) · Accepted for publication in A&A, updated to match final journal version
arxiv created 2014/06/05 · openalex publication_date 2014/06/05 · arxiv updated 2014/09/05 · openalex created_date 2022/10/06 · openalex updated_date 2026/07/30
Context. We studied the size–surface brightness and the size–mass relations of a sample of 16 cluster elliptical galaxies in the mass range ~ 1010−2 × 1011 M⊙, which were morphologically selected in the cluster RDCS J0848+4453 at z = 1.27.