Budget Amount *help |
¥4,680,000 (Direct Cost: ¥3,600,000、Indirect Cost: ¥1,080,000)
Fiscal Year 2016: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2015: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
Fiscal Year 2014: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
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Outline of Final Research Achievements |
We systematically analyzed the X-ray spectra of many active galactic nuclei in the local universe observed with Suzaku and XMM-Newton. We have found that (1) about half of radio galaxies have ultra fast outflows, (2) the mean solid angle of tori increases with luminosity at low luminosities, and (3) a key parameter that determines AGN feedback is the Eddington ratio. By optical spectroscopic observations of ultra-luminous X-ray sources, we have revealed that they are in the supercritical accretion state, ejecting a large amount of gas via disk winds.
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