Budget Amount *help |
¥5,200,000 (Direct Cost: ¥4,000,000、Indirect Cost: ¥1,200,000)
Fiscal Year 2016: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2015: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2014: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2013: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2012: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
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Outline of Final Research Achievements |
The purpose of this work is to detect Recombining plasma (RP) from many SNR, using the Suzaku high spectral capability, and address new scenario of SNR evolution. We found RP from 7 SNRs for the first time, and study the evolutional scenario to produce the RP. Furthermore we detect Cr, Mn, Fe and Ni K-shell line from many SNRs and address the explosion mechanisms, origin of the Galactic diffuse X-ray emission and the origin of the Cosmic Rays.
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