New approach to study of high-energy emission mechanisms of HMXBs
| Project/Area Number |
21540304
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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 | Tokai University |
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Principal Investigator |
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| Co-Investigator(Kenkyū-buntansha) |
NAITOU Tsuguya 山梨学院大学, 経営情報学部, 教授 (50319084)
OKAZAKI Atsuo 北海学園大学, 工学部, 教授 (00185414)
HAYASAKI Kimitake 京都大学, 大学院・理学系研究科, 研究員 (30374218)
NAGATAKI Shigehiro 京都大学, 基礎物理学研究所, 准教授 (60359643)
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| Project Period (FY) |
2009 – 2011
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| Project Status |
Completed (Fiscal Year 2011)
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| Budget Amount *help |
¥4,420,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥1,020,000)
Fiscal Year 2011: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2010: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
Fiscal Year 2009: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
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| Keywords | 高エネルギー宇宙物理 / シミュレーション / 赤外線観測 / 連星系 / 赤外観測 / シミュレーショ |
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| Research Abstract |
We have introduced a 3-d hydrodynamic simulations in modeling a Gamma-ray binary, PSRB1259-63 to study emission mechanisms. Our NIR observations of the system constrain the model of the disk of the massive star.
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Report
(4 results)
Research Products
(71 results)
