| Co-Investigator(Kenkyū-buntansha) |
TANABE Toshihiko 東京大学, 大学院・理学系研究科, 助教 (90179812)
NAKADA Yoshikazu 東京大学, 大学院・理学系研究科, 教授 (80011740)
KANEDA Hidehiro 名古屋大学, 大学院・理学研究科, 准教授 (30301724)
KAWAMURA Akiko 名古屋大学, 大学院・理学研究科, 准教授 (30377931)
ITA Yoshifusa 東北大学, 大学院・理学研究科, 助教 (30392814)
SAKON Itsuki 東京大学, 大学院・理学系研究科, 助教 (70451820)
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| Budget Amount *help |
¥42,250,000 (Direct Cost: ¥32,500,000、Indirect Cost: ¥9,750,000)
Fiscal Year 2009: ¥9,750,000 (Direct Cost: ¥7,500,000、Indirect Cost: ¥2,250,000)
Fiscal Year 2008: ¥10,010,000 (Direct Cost: ¥7,700,000、Indirect Cost: ¥2,310,000)
Fiscal Year 2007: ¥10,660,000 (Direct Cost: ¥8,200,000、Indirect Cost: ¥2,460,000)
Fiscal Year 2006: ¥11,830,000 (Direct Cost: ¥9,100,000、Indirect Cost: ¥2,730,000)
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| Research Abstract |
This research aims to make systematic observations in the infrared region for the Large Magellanic Cloud and nearby galaxies with AKARI, which was launched in 2006 February, and construct a fundamental database from the near-to far-infrared region as well as a point source catalog of the Large Magellanic cloud. Together with these AKARI data, complementary spectroscopic observations with Spitzer of star-forming regions and nearby galaxies were carried out to study material evolution and circulation in galaxies based on systematic observations of the interstellar matter in the various physical conditions.
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