PPT-Roles of Cosmic Rays in Galaxy Clusters

Author : stefany-barnette | Published Date : 2016-06-10

Yutaka Fujita Osaka U Content CRs may be playing more important roles in clusters than you imagine Cosmic ray CR heating of cluster cores Fujita amp Ohira 2011

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Roles of Cosmic Rays in Galaxy Clusters: Transcript

Yutaka Fujita Osaka U Content CRs may be playing more important roles in clusters than you imagine Cosmic ray CR heating of cluster cores Fujita amp Ohira 2011 2012 2013 Fujita Kimura amp Ohira 2013. Weipeng Lin. Shanghai Astronomical Observatory, CAS, China. linwp@shao.ac.cn. Theory of structure formation. Origin. ：. the tiny density deviation from primeval quantum field fluctuation, amplified by gravitational instability. AMS Discoveries Affecting Cosmic-Ray SIG Priorities. Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. AY 17. 10/19/2011. Outline. What is Multi-messenger astronomy?. Photons. Cosmic Rays. Neutrinos. Gravity-Waves. Sample-Return. Outline. What is Multi-messenger astronomy?. Photons. Cosmic Rays. Neutrinos. Andrea . Chiavassa. Universita. ` . degli. . Studi. . di. Torino. Carpathian Summer School of Physics 2012. June 24 – July 7, . Sinaia. , Romania. Most of the material comes from the book:. “. the merger/. sloshing. . cold. front . paradigm. :. A2142 . revisited. by XMM. Mariachiara Rossetti. (Università degli Studi di Milano & IASF Milano). D. . . Eckert. , S. De Grandi, S. . Molendi. . Reionization. . . Chris . Carilli. (. M/N. RAO). Vatican Summer School June 2014. I. Introduction: Cosmic . Reionization. Concept . . Cool gas in z > 6 galaxies: quasar hosts. Constraints on evolution of neutral Intergalactic Medium (IGM). galaxy group, Stephan S. R. Kulkarni. Caltech Optical Observatories. Key Papers. “On Supernovae” Baade & . Zwicky. (1934a). “Cosmic Rays From Supernovae” Baade & . Zwicky. (1934b). “On the Search for Supernovae” . 23.1 Our Parent Galaxy. 23.2 Measuring the Milky Way. Early “Computers”. 23.3 Galactic Structure. 23.4 The Formation of the Milky Way. 23.5 Galactic Spiral Arms. Density Waves. 23.6 The Mass of the Milky Way Galaxy. Galaxy Morphology and Environment. Main relation – . E’s more common in clusters than field. f(E. ) = fraction of ellipticals . f(Sp. ) = fraction of spirals. regular, symmetric cluster – . f(E. Here’s the mystery story we’ll unfold…. Fuzzy blobs in the sky – new solar systems, or “galaxies”?. Observational tests. Herschel’s map of the “universe” . (what we today know as just our Galaxy). Plasma. . Astrophysics. Roger . Blandford. Paul Simeon. Yajie. Yuan. KIPAC. Stanford. 27 i 2012. AronsFest. 2. Describing Cosmic Plasma. Fluid description. P. , . . , . v. , B…. Magneto Fluid Dynamics . Eun-Suk. . Seo. Inst. for Phys. Sci. & Tech. and . Department of Physics. University of Maryland. AAS HEAD meeting, Chicago, IL, 19 August 2014. w. ith edits & voice from . Angela V. Olinto. X Rays. Are electromagnetic radiations having wavelength of order of 1. Are highly energetic radiations which are emitted when energetic electrons are made to incident on a metallic target.. Were discovered by German Physicist W.C. Roentgen in1895..

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