Nearby groups and clusters provide laboratories to study the impact of environment on the properties of member galaxies, including gas content, star formation rates, morphology, and nuclear activity. This meeting focused on the observed gas content and star formation properties of galaxies in groups and clusters in the local universe, and the current theoretical understanding of the dominant physical mechanisms at work.
PDF of presentations are linked from the Conference Schedule.
Supported in part by the Skidmore Union Network under National Science Foundation Grant No. 0820032 and by Siena College.
Gas and Star Formation Properties of Group and Cluster Galaxies
X-ray Properties of Groups and Clusters
Connection with High-z Groups and Clusters
Dwarf Galaxies in Groups and Clusters
Ongoing and Future Surveys