| Budget Amount *help |
¥17,160,000 (Direct Cost: ¥13,200,000、Indirect Cost: ¥3,960,000)
Fiscal Year 2019: ¥4,810,000 (Direct Cost: ¥3,700,000、Indirect Cost: ¥1,110,000)
Fiscal Year 2018: ¥4,940,000 (Direct Cost: ¥3,800,000、Indirect Cost: ¥1,140,000)
Fiscal Year 2017: ¥5,070,000 (Direct Cost: ¥3,900,000、Indirect Cost: ¥1,170,000)
Fiscal Year 2016: ¥2,340,000 (Direct Cost: ¥1,800,000、Indirect Cost: ¥540,000)
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| Outline of Final Research Achievements |
We have theoretically studied the active galactic nucleus (AGN), which consists of a supermassive black hole (SMBHs) at the centre of many galaxies. In particular, we combined the multi-dimensional radiative magnetohydrodynamic calculations and multi-wavelength pseudo-observations. We compared the numerical results with the multi-wavelength observational studies to understand1) the physical origin of the obscuring tori, 2) physics and parameters that determine the structure of the ISM around SMBH, 3) mass accretion processes and the origin of the buried AGN. We have succeeded in developing a theoretical model (radiation-driven fountain model) that explains the observational results of nearby AGNs. These studies are useful to understand the cosmological evolution of quasars and buried AGNs.
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