A New Scenario of the SNR evolution using the Recombining Plasma
| Project/Area Number | 24540229 |
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| Research Category |
Grant-in-Aid for Scientific Research (C)
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| Allocation Type | Multi-year Fund |
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| Section | 一般 |
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| Research Field |
Astronomy
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| Research Institution | Kyoto University |
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Principal Investigator |
Katsuji Koyama 京都大学, 理学研究科, 名誉教授 (10092206)
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| Project Period (FY) |
2012-04-01 – 2017-03-31
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| Project Status |
Completed(Fiscal Year 2016)
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| Budget Amount *help |
¥5,200,000 (Direct Cost : ¥4,000,000、Indirect Cost : ¥1,200,000)
Fiscal Year 2016 : ¥1,040,000 (Direct Cost : ¥800,000、Indirect Cost : ¥240,000)
Fiscal Year 2015 : ¥1,040,000 (Direct Cost : ¥800,000、Indirect Cost : ¥240,000)
Fiscal Year 2014 : ¥1,040,000 (Direct Cost : ¥800,000、Indirect Cost : ¥240,000)
Fiscal Year 2013 : ¥1,040,000 (Direct Cost : ¥800,000、Indirect Cost : ¥240,000)
Fiscal Year 2012 : ¥1,040,000 (Direct Cost : ¥800,000、Indirect Cost : ¥240,000)
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| Keywords | 超新星残骸 / エックス線 / 過電離プラズマ / 元素組成 / 宇宙線起源 / 超新星 / Ｘ線スペクトル / 電離非平衡プラズマ / 重元素組成 / 非等方爆発 / 未電離プラズマ |
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| Outline of Final Research Achievements |
The purpose of this work is to detect Recombining plasma (RP) from many SNR, using the Suzaku high spectral capability, and address new scenario of SNR evolution. We found RP from 7 SNRs for the first time, and study the evolutional scenario to produce the RP. Furthermore we detect Cr, Mn, Fe and Ni K-shell line from many SNRs and address the explosion mechanisms, origin of the Galactic diffuse X-ray emission and the origin of the Cosmic Rays.
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Report
(6results)
Research Products
(32results)
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[Journal Article] Evidence for Thermal X-Ray Line Emission from the Synchrotron-dominated Supernova Remnant RX J1713.7-39462015
Author(s)
Katsuda, Satoru; Acero, Fabio; Tominaga, Nozomu; Fukui, Yasuo; Hiraga, Junko S.; Koyama, Katsuji; Lee, Shiu-Hang; Mori, Koji; Nagataki, Shigehiro; Ohira, Yutaka; and 7 coauthors
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Journal Title
Astrophysical Journal
Volume : 814
Pages : 1-11
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research / Acknowledgement Compliant
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[Journal Article] Kepler's Supernova : An Overluminous Type Ia Event Interacting with a Massive Circumstellar Medium at a Very Late Phase2015
Author(s)
Katsuda, Satoru ; Mori, Koji ; Maeda, Keiichi ; Tanaka, Masaomi ; Koyama, Katsuji ; Tsunemi, Hiroshi ; Nakajima, Hiroshi ; Maeda, Yoshitomo ; Ozaki, Masanobu ; Petre, Robert
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Journal Title
Astrophysical Journal
Volume : 808
Pages : 1-14
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research / Acknowledgement Compliant
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[Journal Article] A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from the Enhanced Abundances of Nickel and Manganese2015
Author(s)
Yamaguchi, Hiroya; Badenes, Carles; Foster, Adam R.; Bravo, Eduardo; Williams, Brian J.; Maeda, Keiichi; Nobukawa, Masayoshi; Eriksen, Kristoffer A.; Brickhouse, Nancy S.; Petre, Robert; Koyama, Katsuji
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Journal Title
Astrophysical Joarnal
Volume : 801
Pages : 31-37
DOI
Related Report
Peer Reviewed / Acknowledgement Compliant
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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
Pages : 648-648
DOI
Related Report
Peer Reviewed / Open Access / Acknowledgement Compliant
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