Suzaku Observation of the Galactic Diffuse(Chapter 4. Warm and Hot IntraGalactic Medium, The Extreme Universe in the Suzaku Era)

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概要

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• The CCD camera (XIS) onboard Suzaku functions properly since its launch. The energy covered is from 0.2keV to 12keV with low background condition. So far, we have observed various emission lines including C and N. We can determine the abundances of C, N and O, independently. The high performance of Suzaku enables us to obtain the evidence of the charge-exchange process. We will summarize the latest Suzaku results on the galactic diffuse category, particularly on the thermal emission.

• 理論物理学刊行会の論文
• 2007-12-19

著者

• Tsunemi Hiroshi

  Graduate School Of Science Earth And Space Science Osaka University

関連論文

• Search for Sc-K Line Emission from RX J0852.0-4622 Supernova Remnant with Suzaku
• Suzaku Observation of the Galactic Diffuse(Chapter 4. Warm and Hot IntraGalactic Medium, The Extreme Universe in the Suzaku Era)

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