2006/07/19 by A. G. Bedregal, Alfonso Aragón‐Salamanca, A. Aragón-Salamanca +3 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Elliptical galaxy #Fornax Cluster #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy formation and evolution #Kinematics #Observatory #Physics #Spectral line #Spectrograph #Stellar, planetary, and galactic studies #Telescope #Tully–Fisher relation #Velocity dispersion #Very Large Telescope #astro-ph
paper · pdf · doi:10.1111/j.1365-2966.2006.10829.x
published as Mon.Not.Roy.Astron.Soc.371:1912-1924,2006 · 17 pages, 13 figures, 3 tables, accepted in MNRAS
arxiv created 2006/07/19 · openalex publication_date 2006/08/21 · arxiv updated 2009/12/01 · openalex created_date 2020/11/23 · openalex updated_date 2026/08/05
We have obtained long-slit spectroscopy for a sample of nine S0 galaxies in the Fornax Cluster using the FORS2 spectrograph at the 8.2-m European Southern Observatory (ESO) Very Large Telescope (VLT). From these data, we have extracted the kinematic parameters, comprising the mean velocity, velocity dispersion and higher moment h3 and h4 coefficients, as a function of position along the major axes of these galaxies. Comparison with published kinematics indicates that earlier data are often limited by their lower signal-to-noise ratio and relatively poor spectral resolution. The greater depth and higher dispersion of the new data mean that we reach well beyond the bulges of these systems, probing their disc kinematics in some detail for the first time. Qualitative inspection of the results for individual galaxies shows that they are not entirely simple systems, perhaps indicating a turbulent past. None the less, we are able to derive reliable circular velocities for most of these systems, which points the way towards a study of their Tully–Fisher relation. This study, along with an analysis of the stellar populations of these systems out to large galactocentric distances, will form the bases of future papers exploiting these new high-quality data, hopefully shedding new light on the evolutionary history of these systems.