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Suzaku Observations of TeV Galactic sources
https://jaxa.repo.nii.ac.jp/records/4935
https://jaxa.repo.nii.ac.jp/records/49359ee6e9f6-0b39-4cc3-a21d-40a445004723
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
64574003.pdf (310.1 kB)
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| Item type | 会議発表論文 / Conference Paper(1) | |||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| 公開日 | 2015-03-26 | |||||||||
| タイトル | ||||||||||
| タイトル | Suzaku Observations of TeV Galactic sources | |||||||||
| 言語 | en | |||||||||
| 言語 | ||||||||||
| 言語 | eng | |||||||||
| キーワード | ||||||||||
| 言語 | en | |||||||||
| 主題Scheme | Other | |||||||||
| 主題 | acceleration of particles - shock waves - ISM: X-rays | |||||||||
| 資源タイプ | ||||||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||||||
| 資源タイプ | conference paper | |||||||||
| 著者 |
馬場, 彩
× 馬場, 彩
× Bamba, Aya
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| 著者所属 | ||||||||||
| 宇宙航空研究開発機構宇宙科学研究本部 | ||||||||||
| 著者所属（英） | ||||||||||
| en | ||||||||||
| Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA) | ||||||||||
| 出版者 | ||||||||||
| 出版者 | 宇宙航空研究開発機構 | |||||||||
| 出版者（英） | ||||||||||
| 出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||||||
| 書誌情報 |
宇宙航空研究開発機構特別資料: en : JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 10-13, 発行日 2010-02-26 |
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| 会議概要（会議名, 開催地, 会期, 主催者等）（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||||||
| 抄録（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | It has been one of the biggest problems what is the origin of Galactic cosmic-rays. Previous X-ray surveys found several supernova remnants (SNRs) which have synchrotron X-rays, although the number is too small to account for the total energy of cosmic-rays. HESS, on the other hand, discovered tens of new unidentified (TeV unID) sources on the Galactic plane, which could be the main contributors of the Galactic cosmic-rays. However, we need follow-up observations to understand the nature of these TeV unID sources. Suzaku has already done deep follow-up observations of most TeV unIDs and pin-pointed their nature. Only one TeV inID source is categorized as an SNR, whereas several sources are identified as pulsar wind nebulae (PWNe). In this paper, we will discuss on what is the main contributors of TeV unID sources and Galactic cosmic-rays. We also discuss on GeV observations of TeV unIDs and future aspects. | |||||||||
| 内容記述（英） | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||||||
| ISSN | ||||||||||
| 収録物識別子タイプ | ISSN | |||||||||
| 収録物識別子 | 1349-113X | |||||||||
| 書誌レコードID | ||||||||||
| 収録物識別子タイプ | NCID | |||||||||
| 収録物識別子 | AA11984031 | |||||||||
| 資料番号 | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | 資料番号: AA0064574003 | |||||||||
| レポート番号 | ||||||||||
| 内容記述タイプ | Other | |||||||||
| 内容記述 | レポート番号: JAXA-SP-09-008E | |||||||||
