Seminar Title |
Clusters of Galaxies in X-ray |
Speaker: |
Dr. SU Yuanyuan |
Affiliation: |
(University of California, Irvine) |
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When: |
Monday morning , Mar. 24th , 10:00 a.m |
Where: |
Room 619, Office Block, 2 West Beijing Road (PMO, CAS) |
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Welcome to Attend |
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( PMO Academic Committee & Academic Circulating committee) |
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| Abstract The standard model of cosmology, a universe dominated by cold dark matter, directly predicts that bounded systems on various scales -- galaxies, groups of galaxies, and clusters of galaxies -- evolved from a near-uniform Big Bang through hierarchical formation. Such a scenario naturally gives rise to questions such as how well can self-similarity hold for systems on different scales and what is the role played by baryon physics in their evolution. 90% of the baryons in galaxy groups and clusters are in the form of hot gas emitting in X-rays through bremsstrahlung radiation. Together, three ongoing major X-ray missions (Chandra, XMM-Newton and Suzaku), with different advantages to complement each other, enable us to study various physics and over a wide range of physical parameters. I will talk about recent studies of baryon physics in clusters and groups, such as gas fraction, gaseous clumpiness, AGN feedback, ram pressure, and metal enrichment.
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