2008/04/22 by Igor Chilingarian, Veronique Cayatte, V. Cayatte +11
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Biology #Cluster (spacecraft) #Context (archaeology) #Dwarf galaxy #Elliptical galaxy #Fornax Cluster #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Luminosity #Luminosity function #Paleontology #Physics #Stellar, planetary, and galactic studies #Virgo Cluster #astro-ph
paper · pdf · doi:10.1051/0004-6361:20078709
Accepted to A&A, 48 pages, 62 figures, 3 tables. This version contains low-resolution figures. We encourage you to get the full-resolution PDF (16Mb) from http://voplus.obspm.fr/DataCollections/Abell0496/
openalex publication_date 2008/04/22 · arxiv created 2008/05/02 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
Context. The morphology and stellar populations of low-luminosity early-type galaxies in clusters have until now been limited to a few relatively nearby clusters such as Virgo or Fornax. Scenarii for the formation and evolution of dwarf galaxies in clusters are therefore not well constrained.