'1 kev' diaporamas de présentation

Study of the Galactic Diffuse X-Ray Emission with the Suzaku Satellite

Study of the Galactic Diffuse X-Ray Emission with the Suzaku Satellite. ???????????. ?????????. COBE/DIRBE ??? 1.25, 2.2, 3.5 ?m. Galactic Diffuse X-Ray Emission (GDXE). ~1 ???. Sgr A *. Sgr A *. ??? b (degree). ?? l (degree). RXTE/PCA 3-20 keV. Revnivtsev et al. 2006.

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Strangeness Nuclear Physics at J-PARC

Strangeness Nuclear Physics at J-PARC. Kyungpook National University May. 26, 2009 Kiyoshi Tanida. Nuclear Physics. Study properties and reactions of nuclei. ~3000 found, >5000 should exist. neutron number. proton number. Why interesting?. I would give you just one example here.

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Antimatter in our Galaxy unveiled by INTEGRAL

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A Review of the Observations: Cluster Cooling Flows 2003

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Search for ? + EC and ECEC processes in 112 Sn

Search for ? + EC and ECEC processes in 112 Sn. 1. A.S. Barabash 1) , Ph. Hubert 2) , A. Nachab 2) and V. Umatov 1) 1) ITEP, Moscow, Russia 2) CNBG, Gradignan, France. Outline. Introduction Experiment Results Conclusion. I. Introduction. 2 ? + , ? + EC and ECEC processes:

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A1309.01

A1309.01. Imaging Parameters. A1309.01. Imaging Parameters. A1309.01. HESSI. A1309.02. HESSI Science Objective. To explore the basic physics of particle acceleration and explosive energy release in Solar Flares. Impulsive Energy Release in the Corona

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Measurement of X rays from X - atom

Measurement of X rays from X - atom. XiX Collaboration Spokesperson: K. Tanida (Kyoto Univ.) 30/June/2006. Collaboration. Kyoto University S. Dairaku, H. Fujimura, K. Imai, S. Kamigaito, K. Miwa, A. Sato, K. Senzaka. K. Tanida (spokesperson), C. J. Yoon Brookhaven National Laboratory

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Marie Machacek Smithsonian Astrophysical Observatory

Probing the Dynamics of Galaxy-Gas Interactions in Groups and Clusters with Chandra and XMM-Newton. Marie Machacek Smithsonian Astrophysical Observatory. IGM Workshop 3/8/2005. Thanks to my collaborators. Christine Jones William R. Forman Paul Nulsen Ralph Kraft

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The Galactic Center Diffuse X-Rays Katsuji Koyama , Kyoto University

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Overview of Results in the MST Reversed-Field Pinch

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Millisecond pulsar population and related high energy phenomena

Millisecond pulsar population and related high energy phenomena. ? ? (NAOC). July 2009, Pulsar Summer School Beijing. Contents. Introduction to millisecond pulsars (MSPs); High energy emissions in MSPs: observations versus theories ;

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Starting Points (Collaboration ; Laboratory ) Magnetic Moment Results with HPGe

Low Energy Neutrino Physics at the Kuo-Sheng Reactor Laboratory Focus of This Talk : Research Program towards Observation of Neutrino-Nucleus Coherent Scattering. Starting Points (Collaboration ; Laboratory ) Magnetic Moment Results with HPGe Physics & Motivations of n N

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Suzaku observations of AGN and synergy with GLAST

Suzaku observations of AGN and synergy with GLAST. PKS1510-089 ( Suzaku ). Jun Kataoka (Tokyo Tech) in collaboration with T.Takahashi ,G.Madejski, T.Kamae, S.Watanabe, M.Ushio, T.Kohmura and Suzaku team. Outline. About Suzaku. - Mission status. - Payloads & advantages.

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Antimatter in our Galaxy unveiled by INTEGRAL

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The s-process in massive stars

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The Magnetic Field of an Isolated Neutron Star from X-ray Cyclotron Absorption Lines

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Crab: the standard X-ray candle with all (modern) X-ray satellites

Crab: the standard X-ray candle with all (modern) X-ray satellites.

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Correlations Between Spectral and LFQPO Timing Parameters

Correlations Between Spectral and LFQPO Timing Parameters. Summary of draft results prepared by Jeff McClintock for MIT Workshop on Magnetized Accretion Disks Based on work by J. McClintock, R. Remillard, M. Rupen A. Levine, C. Bailyn, J. Orosz, V. Dhawan, G. Pooley October 19, 2006.

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A Candidate Neutron Star & Its Association with Sgr A East

High Energy Phenomena in the Galactic Center, Paris, France, June 15, 2005. A Candidate Neutron Star & Its Association with Sgr A East. Sangwook Park. Department of Astronomy & Astrophysics. The Pennsylvania State University. Collaborators: Michael Muno (UCLA) Frederick Baganoff (MIT)

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???? ??? ? X ???

?????? 3C 35 ? ?????????? ???? ( ???? , n-isobe@kusastro.kyoto-u.ac.jp), Gandhi Poshak (ISAS/JAXA), ???? , ??? ( ???? ). ?? with Tango Dancers @ ????????. ???? ??? ? X ???. ??????. ??????? : 3C 35. ???????. 1.4 GHz. ??????????? D = 1 Mpc ????????????? ??? ??????

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