An X-ray study of cosmic ray electrons and positrons from pulsar wind nebulae
Project/Area Number |
24740167
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Research Category |
Grant-in-Aid for Young Scientists (B)
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Allocation Type | Multi-year Fund |
Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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Research Institution | University of Miyazaki |
Principal Investigator |
MORI KOJI 宮崎大学, 工学部, 准教授 (00404393)
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Project Period (FY) |
2012-04-01 – 2015-03-31
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Project Status |
Completed (Fiscal Year 2014)
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Budget Amount *help |
¥4,030,000 (Direct Cost: ¥3,100,000、Indirect Cost: ¥930,000)
Fiscal Year 2014: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2013: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2012: ¥1,690,000 (Direct Cost: ¥1,300,000、Indirect Cost: ¥390,000)
|
Keywords | パルサー星雲 / 宇宙線電子陽電子 / 超新星残骸 / TeV 未同定天体 |
Outline of Final Research Achievements |
Pulsar wind nebulae (PWNe) are known as cosmic electron-positron accelerators. However, it has been unclear how the accelerated electrons and positrons escape from the pulsar and diffuse into surrounding space. Since such high energy particles emit X-ray, X-ray observation is the best probe to tackle this issue. In this study, we performed X-ray observations of the Vela PWN, which is the nearest to us. We found that there is a yet unknown component prevailing almost isotropically in addition to already known complex structure around the pulsar. We also discovered new PWN candidates and estimated a metallicity of the progenitor of Kepler's supernova.
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Report
(4 results)
Research Products
(24 results)
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[Journal Article] X-Ray Ejecta Kinematics of the Galactic Core-Collapse Supernova Remnant G292.0+1.82015
Author(s)
Bhalerao, J., Park, S., Dewey, D., Hughes, J.P., Mori, K., and Lee, J-J.
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Journal Title
The Astrophysical Journal
Volume: 800
Issue: 1
Pages: 65-65
DOI
Related Report
Peer Reviewed
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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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[Journal Article] A Deep Chandra Observation of Oxygen-rich Supernova Remnant B0049-73.6 in the Small Magellanic Cloud2014
Author(s)
Schenck, A., Park, S., Burrows, D.N., Hughes, J.P., Lee, J-J., and Mori, K.
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Journal Title
A Deep Chandra Observation of Oxygen-rich Supernova Remnant B0049-73.6 in the Small Magellanic Cloud
Volume: 791
Issue: 1
Pages: 50-50
DOI
Related Report
Peer Reviewed
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[Journal Article] Asymmetry in the Observed Metal-rich Ejecta of the Galactic Type Ia Supernova Remnant G299.2-2.92014
Author(s)
Post, S., Park, S., Badenes, C., Burrows, D.N., Hughes, J.P., Lee, J-J., Mori, K., and Slane, P.
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Journal Title
The Astrophysical Journal Letters
Volume: 792
Issue: 1
Pages: L20-L20
DOI
Related Report
Peer Reviewed
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[Journal Article] A Suzaku Study of Ejecta Structure and Origin of Hard X-Ray Emission in the Supernova Remnant G156.2+5.72012
Author(s)
Uchida, H., Tsunemi, H., Katsuda, S., Mori, K., Petre, R., and Yamaguchi, H.
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Journal Title
Publications of the Astronomical Society of Japan
Volume: 64
Pages: 61-70
NAID
Related Report
Peer Reviewed
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[Journal Article] Discovery of a Pulsar Wind Nebula Candidate in the Cygnus Loop2012
Author(s)
Katsuda, S., Tsunemi, H., Mori, K., Uchida, H., Petre, R., Yamada, S., and Tamagawa, T.
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Journal Title
The Astrophysical Journal Letters
Volume: 754
Issue: 1
Pages: 7-11
DOI
Related Report
Peer Reviewed
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