Continuum and Line Emissions from the Galactic Ridge and Clusters : Problems of Interpretation and Ways of Solution(Chapter 5. The Galactic Center and Ridge Emissions, The Extreme Universe in the Suzaku Era)

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概要

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• The stochastic acceleration of subrelativistic electrons from background plasma is studied in order to find possible explanation of hard X-ray emission from the Galactic Ridge and galaxy clusters. From our analysis we show that the energy supply required to produce this emission is much less than it was obtained in the framework of previous models.

• 理論物理学刊行会の論文
• 2007-12-19

著者

• KUO Ping-Hung

  Institute of Astronomy, National Central University

• IP Wing-Huen

  Institute of Astronomy, National Central University

• Ip Wing-huen

  Institute Of Astronomy National Central University

• Kuo Ping-hung

  Institute Of Astronomy National Central University

• Masai Kuniaki

  Tokyo Metropolitan Univ. Tokyo

• Masai Kuniaki

  Tokyo Metropolitan University

• DOGIEL Vladimir

  P. N. Lebedev Institute of Physics

• KO Che

  Institute of Astronomy, National Central University

• HWANG Chorng-Yuan

  Institute of Astronomy, National Central University

• Ko Che

  Institute Of Astronomy National Central University

• Hwang Chorng-yuan

  Institute Of Astronomy National Central University

• Kuo Ping‐hung

  National Central Univ. Chung‐li Twn

関連論文

• New CTI Correction Method for Spaced-Row Charge Injection of the Suzaku X-Ray Imaging Spectrometer
• A multiband study of the optically dark GRB 051028
• Suzaku Observation of the Southeastern Rim of the Cygnus Loop
• Another Abundance Inhomogeneity in the South East Limb of the Cygnus Loop
• Abundance Inhomogeneity in the Northern Rim of the Cygnus Loop
• Ejecta Distributions of Heavy Elements in the Cygnus Loop
• Suzaku Observations across the Cygnus Loop from the Northeastern to the Southwestern Rim
• Continuum and Line Emissions from the Galactic Ridge and Clusters : Problems of Interpretation and Ways of Solution(Chapter 5. The Galactic Center and Ridge Emissions, The Extreme Universe in the Suzaku Era)
• A Shape-and-Density Model of the Putative Binary EKBO 2001 QG_
• X-Ray Spectrum of a Peculiar Supernova Remnant, G359.1-0.5
• Core Structure of Intracluster Gas : Isothermal Hydrostatic Equilibrium
• First Detection of Ar-K Line Emission from the Cygnus Loop

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