2006/11/20 by M. Hilker, H. Baumgardt, L. Infante +3
Physics and Astronomy · #Astronomy and Astrophysical Research #Dark matter #Dwarf galaxy #Dwarf galaxy problem #Dwarf spheroidal galaxy #Elliptical galaxy #Fornax Cluster #Galaxies: Formation, Evolution, Phenomena #Galaxy #Globular cluster #Scientific Research and Discoveries #astro-ph
paper · pdf · doi:10.1051/0004-6361:20066429
14 pages, 11 figures, accepted for publication in Astronomy & Astrophysics
openalex publication_date 2006/11/20 · arxiv created 2006/12/18 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Aims.We determine masses and mass-to-light ratios of five ultra-compact dwarf galaxies (UCDs) and one dwarf elliptical nucleus in the Fornax cluster from high resolution spectroscopy. We examine whether they are consistent with pure stellar populations or whether dark matter is needed to explain their masses.