Budget Amount *help |
¥2,730,000 (Direct Cost: ¥2,100,000、Indirect Cost: ¥630,000)
Fiscal Year 2016: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2015: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
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Outline of Final Research Achievements |
We have performed large-scale numerical simulations and multi-wavelength radiation transfer calculations. Our simulations show evolution from first galaxies to massive galaxies, and their observational properties. Large amounts of gas accrete onto galaxies, and make massive galactic disks in an over-dense region. The massive galaxies become bright at infrared band due to dust thermal emission in the galactic disk. We also derive the conditions for formations of Population III star clusters and massive black holes in first galaxies by using analytical models.
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