Abstract
Results of a set of N-body simulations of groups of galaxies and their comparison with observations are reported. A preliminary analysis of the theoretical and observed velocity dispersion distributions indicates a basic discrepancy possibly related with projection effects and the presence of interlopers.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.