Invited Speakers
- July 12-14, 2011
- Tuesday, July 12
- Morning - General Overview
- I. Cluster Structure Since 2000, What Has Chandra Seen and How Has it Changed Our Views?
- 9:00-9:30
- Chandra's Clear View of the Structure of Clusters
- II. Cluster and Group Physics - Gas Dynamics, Transport Properties, Outstanding Questions
- 11:00-11:30
- X-ray Surface Brightness Fluctuations and ICM Physics
- Afternoon - AGN Feedback
- III. Observational Overview to AGN Feedback
- 2:00-2:30 Megan Donahue
- AGN Feedback and Cluster Environment
- IV. Theory of Feedback/Numerical Simulations
- 4:15-4:45
- Cosmological Simulations of AGN Feedback in Groups and Clusters: Implementation, Results and Uncertainties
- Wednesday, July 13
- Morning - Evolution of Groups and Clusters
- V. Observational Overview
- 9:00-9:30
- Substructures in Galaxy Clusters
- VI. Simulations
- 11:30-12:00
- Magnetic Fields, Turbulence and Cosmic Rays in Galaxy Clusters
- Afternoon - Masses, Baryons, and Metals
- VII. Masses, Baryons, and Metals (Part 1)
- 2:00-2:30
- Baryons in the Outskirts of the Nearest Brightest Galaxy Clusters
- VIII. Masses, Baryons, and Metals (Part 2)
- 4:30-5:00
- Galaxy, Group and Cluster Mass Profiles from Small Scales out to the Virial Radius
- Thursday, July 14
- Morning
- IX. Multiphase Gas in Clusters and Groups
- 9:00-9:30
- The Cold Gas in Cluster Cores - So Much Progress in the Chandra Era!
- X. Conference summary/panel discussion
- 11:15-12:30
Last modified: 06/13/11