| Project/Area Number |
19540274
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Single-year Grants |
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| Section | 一般 |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | The University of Tokyo |
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Principal Investigator |
KIFUNE Tadashi The University of Tokyo, 宇宙線研究所, 名誉教授 (40011621)
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| Co-Investigator(Kenkyū-buntansha) |
吉越 貴紀 東京大学, 宇宙線研究所, 准教授 (30322366)
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| Co-Investigator(Renkei-kenkyūsha) |
YOSHIKOSHI Takanori 東京大学, 宇宙線研究所, 准教授 (30322366)
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| Project Period (FY) |
2007 – 2010
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| Project Status |
Completed (Fiscal Year 2010)
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| Budget Amount *help |
¥3,250,000 (Direct Cost: ¥2,500,000、Indirect Cost: ¥750,000)
Fiscal Year 2010: ¥520,000 (Direct Cost: ¥400,000、Indirect Cost: ¥120,000)
Fiscal Year 2009: ¥780,000 (Direct Cost: ¥600,000、Indirect Cost: ¥180,000)
Fiscal Year 2008: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2007: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
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| Keywords | 超高エネルギーガンマ線 / 宇宙線 / 宇宙線の起源 / 粒子天体物理学 / 宇宙の非熱過程 / 宇宙線の伝播 / 超新星残骸 / 活動銀河中心核 / ガンマ線 / 宇宙の超高エネルギー現象 |
|---|
| Research Abstract |
The current status of observational study of very high energy gamma rays from various astronomical objects, established recently as one area of astrophysics after the efforts extending for almost half a century, was discussed and our understandings of the whole view of very high energy gamma ray astronomy were summarized as a review paper by a collaborative work with three other colleagues who are working in and leading this field in Europe and United States. In addition, the present data and their interpretation were discussed and analyzed between gamma rays from Galactic sources and extended emission from Galactic plane.
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