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Special Session 2: Cosmic Evolution of Groups and Clusters

Published online by Cambridge University Press:  05 March 2015

J. M. Vrtilek  and
L. P. David
J. M. Vrtilek
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA email: [email protected]
L. P. David
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA, email: [email protected]
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Abstract

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During the past decade observations across the electromagnetic spectrum have led to broad progress in the understanding of galaxy clusters and their far more abundant smaller siblings, groups. From the X-rays, where Chandra and XMM have illuminated old phenomena such as cooling cores and discovered new ones such as shocks, cold fronts, bubbles and cavities, through rich collections of optical data (including vast and growing arrays of redshifts), to the imaging of AGN outbursts of various ages through radio observations, our access to cluster and group measurements has leaped forward, while parallel advances in theory and modeling have kept pace.

This Special Session offered a survey of progress to this point, an assessment of outstanding problems, and a multiwavelength overview of the uses of the next generation of observatories. Holding the symposium in conjuction with the XXVIIIth General Assembly provided the significant advantage of involving not only a specialist audience, but also interacting with a broad cross-section of the world astronomical community.

Keywords

black hole physicsgalaxies: clusters: generalgalaxies: cooling flowsgalaxies: evolutiongalaxies: intergalactic mediumgalaxies: jets
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 289 - 314
Copyright
Copyright © International Astronomical Union 2015 

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