| Budget Amount *help |
¥3,250,000 (Direct Cost: ¥2,500,000、Indirect Cost: ¥750,000)
Fiscal Year 2017: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2016: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2015: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
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| Outline of Final Research Achievements |
AGN outflow wind, a gas stream from the accretion disk of quasar central engines that are accelerated by radiation pressure, shows time variability, although its origin is not clearly understood. We verified one of the most plausible scenarios for the variability (variability ionization scenario; VIS) through unique observations. Our observations suggest a) variability pattern in outflow wind and quasar luminosity are synchronized and b) an outflow wind has the internal structure whose physical scale is smaller than separation distance between sightlines of two lensed images of quasars. These results support the VIS scenario with a self-shielding effect as an additional mechanism, although the gas motion of outflow wind could partially contribute to the change of outflow wind.
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