A Study of Formation Process of SNRs with X-ray Spectrometers
| Project/Area Number |
26800102
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Multi-year Fund |
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| Research Field |
Astronomy
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| Research Institution | Kyoto University |
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Principal Investigator |
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| Project Period (FY) |
2014-04-01 – 2017-03-31
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| Project Status |
Completed (Fiscal Year 2016)
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| Budget Amount *help |
¥3,380,000 (Direct Cost: ¥2,600,000、Indirect Cost: ¥780,000)
Fiscal Year 2016: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2015: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2014: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
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| Keywords | 超新星残骸 / X線天文 |
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| Outline of Final Research Achievements |
We published several papers for X-ray studies of SNRs with spectrometers during the research period. We also developed the soft X-ray imager (SXI) onboard ASTRO-H (Hitomi), which was successfully launched on February 2016. Although Hitomi was lost by an accident of the attitude control system, we had observed several celestial sources before its lost and confirmed the in-orbit performance of the instruments.
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Report
(4 results)
Research Products
(21 results)
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[Journal Article] Suzaku discovery of Fe K-shell line from the O-rich SNR G292.0+1.82014
Author(s)
Kamitsukasa, Fumiyoshi; Koyama, Katsuji; Tsunemi, Hiroshi; Hayashida, Kiyoshi; Nakajima, Hiroshi; Takahashi, Hiroaki; Ueda, Shutaro; Mori, Koji; Katsuda, Satoru; Uchida, Hiroyuki
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Journal Title
Pub. Astr. Soc. Japan
Volume: 66-3
Issue: 3
Pages: 648-648
DOI
NAID
Related Report
Peer Reviewed / Open Access
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