Globular Clusters and Dark Matter (sub) Halos

Tuesday, May 24, 2022 - 11:00am
Prof. Ray Carlberg (University of Toronto)

Decades of observational data and careful modeling show that stars dominate the gravitational field of the inner 2-3 half-mass radii of globular clusters.

Galaxies Evolution in Cluster Cores and Outskirts

Tuesday, May 31, 2022 - 11:00am
Prof. Louise Edwards (Cal Poly SLO)

When and how does environment impact the evolution of galaxies? We will approach this question by considering two extreme environments. First: The cores of massive clusters. Here, the largest, reddest galaxies of the local universe are found, Brightest Cluster Galaxies (BCGs).


Tuesday, June 7, 2022 - 11:00am
Dr. Ivanna Escala (Carnegie Observatories)

TBD **in person**

Friday, October 21, 2022 - 2:00pm to 3:00pm
Aayush Saxena (UCL)