Satellite galaxies in nearby groups of galaxies
classification
🌌 astro-ph.GA
keywords
galaxiesgroupssatellitenearbyanalyseapproximateddifferentdispersion
read the original abstract
We analyse distribution, kinematics and star-formation (SF) properties of satellite galaxies in three different samples of nearby groups. We find that studied groups are generally well approximated by low-concentration NFW model, show a variety of LOS velocity dispersion profiles and signs of SF quenching in outskirts of dwarf satellite galaxies.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.