Pioneering high-resolution X-ray spectroscopy of supernova remnants using dispersive spectrometers and the calorimeter onboard ASTRO-H
Project/Area Number |
25800119
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Research Category |
Grant-in-Aid for Young Scientists (B)
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Allocation Type | Multi-year Fund |
Research Field |
Astronomy
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Research Institution | Japan Aerospace EXploration Agency (2014-2015) Institute of Physical and Chemical Research (2013) |
Principal Investigator |
Katsuda Satoru 国立研究開発法人宇宙航空研究開発機構, 宇宙科学研究所, 宇宙航空プロジェクト研究員 (50611034)
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Project Period (FY) |
2013-04-01 – 2016-03-31
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Project Status |
Completed (Fiscal Year 2015)
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Budget Amount *help |
¥4,030,000 (Direct Cost: ¥3,100,000、Indirect Cost: ¥930,000)
Fiscal Year 2015: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2014: ¥1,300,000 (Direct Cost: ¥1,000,000、Indirect Cost: ¥300,000)
Fiscal Year 2013: ¥1,430,000 (Direct Cost: ¥1,100,000、Indirect Cost: ¥330,000)
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Keywords | 超新星残骸 / X線精密分光 / X線観測 / XMM-Newton / 分散分光器 / X線天文学 / 精密分光 |
Outline of Final Research Achievements |
It was generally thought that XMM-Newton’s reflection grating spectrometer (RGS) is applicable only for point-like sources. However, in this research, we have successfully demonstrated that the RGS can provide high-resolution spectra for compact supernova remnants (SNRs) like Kepler’s SNR and SNR 0509-67.5 and compact features in large SNRs such as Puppis A and the Cygnus Loop. The outcomes include establishing charge-exchange X-ray emission in X-ray spectra, revealing 3D geometries of supernova ejecta, and the discovery of N-rich circumstellar medium. These are all new to X-ray astronomy and are scientifically important. In addition, inspired by this X-ray high-resolution spectroscopy, we initiated new high-resolution spectroscopy of SNRs in optical and extreme ultraviolet wavelengths.
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Report
(4 results)
Research Products
(21 results)
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[Journal Article] Spatially Resolved Spectroscopy of a Balmer-dominated Shock in the Cygnus Loop: An Extremely Thin Cosmic-Ray Precursor?2016
Author(s)
S. Katsuda, K. Maeda, Y. Ohira, Y. Yatsu, K. Mori, W. Aoki, K. Morihana, J. C. Raymond, P. Ghavamian, J.-J. Lee, J. Shimoda, R. Yamazaki
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Journal Title
The Astrophysical Journal Letters
Volume: 819
Issue: 2
Pages: 1-6
DOI
Related Report
Peer Reviewed / 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
ApJ
Volume: 808
Issue: 1
Pages: 1-14
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research / Acknowledgement Compliant
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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
ApJ
Volume: 814
Issue: 1
Pages: 1-11
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research / Acknowledgement Compliant
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