Magnetic Bubbles in Galaxy Clusters
arXiv:astro-ph/0310708
Abstract
I discuss Chandra X-ray Observatory measurements of cavities in galaxy clusters and their implications for heating the intracluster gas. The emerging paradigm for cooling flows has important implications for understanding self-regulated galaxy formation.
Four pages. Contributed paper, Carnegie Observatories Centennial Symposium "Clusters of Galaxies: Probes of Cosmological Structure and Galaxy Evolution ed. J.S. Mulchaey, A. Dressler, and Oemler