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Observational estimates of the size of structures in the CGM

How do we determine the physical scale of column density variations in the atmospheres of galaxies?

Published onMar 23, 2022
Observational estimates of the size of structures in the CGM

This 27-minute video tutorial from Chris Howk (University of Notre Dame) discusses observational studies of the physical scale of gas structures in the interstellar and circumgalactic media of galaxies. It was presented initially as a contribution to the 2021 program on Fundamentals of Galactic Halos hosted by the Kavli Institute for Theoretical Physics.

Tutorial: Observational Constraints on CGM Cloud Sizes - Chris Howk

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