| Budget Amount *help |
¥4,420,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥1,020,000)
Fiscal Year 2015: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2014: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2013: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2012: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
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| Outline of Final Research Achievements |
The structure of magnetosphere of a black hole is studied to understand the high-energy astrophysical phenomena in active galactic nuclei and some compact X-ray sources. Such high-energy phenomena are due to a massive black hole with magnetized plasma accretion, where the effects of strong gravity (i.e., the general relativistic effects) have a crucial role in the system around the black hole. I and collaborators make a project to detect some information about the black hole's curved spacetime by radio VLBI observation and near-infrared observation.
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