›CGM BERLIN 2019

The goal of this meeting is to bring together a focused group of experts (~40, see below) who are actively working on the circumgalactic medium, from both the theoretical and observational perspectives, to discuss recent advances on the following topics:

-What is the structure and properties of the CGM from sub-parsec to halo scales, and what are the most important physical mechanisms at play?
-How are galaxies, gas flows, and the CGM related?
-Where has the comparison of observations and theory produced insight, where are we still falling short, and what are the next steps?

We plan to address these questions and related CGM/outflows themes through a number of talks and discussions.