Magnetic Bubbles in Galaxy Clusters

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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

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http://salesiana.dossiersoluciones.com/handle/123456789/6858

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0310708
 http://arxiv.org/abs/astro-ph/0310708

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arXiv