WEKO3
アイテム
{"_buckets": {"deposit": "d6c0fabd-8756-482e-aa4c-63ea9d1a737f"}, "_deposit": {"created_by": 1, "id": "4951", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "4951"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00004951", "sets": ["948", "1891"]}, "author_link": ["22797", "22798"], "item_5_biblio_info_10": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2010-02-26", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "51", "bibliographicPageStart": "50", "bibliographicVolumeNumber": "JAXA-SP-09-008E", "bibliographic_titles": [{"bibliographic_title": "宇宙航空研究開発機構特別資料:"}, {"bibliographic_title": "JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H", "bibliographic_titleLang": "en"}]}]}, "item_5_description_15": {"attribute_name": "会議概要(会議名, 開催地, 会期, 主催者等)(英)", "attribute_value_mlt": [{"subitem_description": "The 3rd Suzaku international Conference \"Energetic Cosmos : from Suzaku to ASTRO-H\" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan", "subitem_description_type": "Other"}]}, "item_5_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "The spectral energy distribution from the X-ray to the very high energy regime (\u003e 100 GeV) has been investigated for the gamma-ray binary system PSR B1259-63/SS2883 as a function of orbital phase within the framework of a simple model of a pulsar wind nebula. The emission model is based on the synchrotron radiation process for the X-ray regime and the inverse Compton scattering process boosting stellar photons from the Be star companion to the very high energy (100GeV-TeV) regime. With this model, the observed temporal behavior can, in principle, be used to probe the pulsar wind properties at the shock as a function of the orbital phase.", "subitem_description_type": "Other"}]}, "item_5_description_19": {"attribute_name": "内容記述(英)", "attribute_value_mlt": [{"subitem_description": "Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science", "subitem_description_type": "Other"}]}, "item_5_description_32": {"attribute_name": "資料番号", "attribute_value_mlt": [{"subitem_description": "資料番号: AA0064574019", "subitem_description_type": "Other"}]}, "item_5_description_33": {"attribute_name": "レポート番号", "attribute_value_mlt": [{"subitem_description": "レポート番号: JAXA-SP-09-008E", "subitem_description_type": "Other"}]}, "item_5_publisher_8": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "宇宙航空研究開発機構"}]}, "item_5_publisher_9": {"attribute_name": "出版者(英)", "attribute_value_mlt": [{"subitem_publisher": "Japan Aerospace Exploration Agency (JAXA)"}]}, "item_5_source_id_21": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "1349-113X", "subitem_source_identifier_type": "ISSN"}]}, "item_5_source_id_24": {"attribute_name": "書誌レコードID", "attribute_value_mlt": [{"subitem_source_identifier": "AA11984031", "subitem_source_identifier_type": "NCID"}]}, "item_5_text_35": {"attribute_name": "JAXAカテゴリ", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ: 特別資料"}]}, "item_5_text_40": {"attribute_name": "jaxa出版物種類", "attribute_value_mlt": [{"subitem_text_value": "jaxa出版物種類: SP"}]}, "item_5_text_43": {"attribute_name": "DSpaceコレクション番号", "attribute_value_mlt": [{"subitem_text_value": "DSpaceコレクション番号: 7"}]}, "item_5_text_7": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "Department of Physics, University of Hong Kong"}, {"subitem_text_language": "en", "subitem_text_value": "Academia Sinica Institute of Astrophysics and Astronomy-TIARA"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Takata, Jumpei", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "22797", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Taam, Ronald E.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "22798", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2020-01-16"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "64574019.pdf", "filesize": [{"value": "189.0 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 189000.0, "url": {"label": "64574019.pdf", "url": "https://jaxa.repo.nii.ac.jp/record/4951/files/64574019.pdf"}, "version_id": "db7da5dc-4715-4600-a1a9-e5251cf33987"}]}, "item_keyword": {"attribute_name": "キーワード", "attribute_value_mlt": [{"subitem_subject": "acceleration of particles - radiation mechanisms: non-thermal - gamma rays: theory - Xrays: binaries - pulsars: individual (PSR B1259-63)", "subitem_subject_language": "en", "subitem_subject_scheme": "Other"}]}, "item_language": {"attribute_name": "言語", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "資源タイプ", "attribute_value_mlt": [{"resourcetype": "conference paper", "resourceuri": "http://purl.org/coar/resource_type/c_5794"}]}, "item_title": "Probing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Probing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["948", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/4951", "pubdate": {"attribute_name": "公開日", "attribute_value": "2015-03-26"}, "publish_date": "2015-03-26", "publish_status": "0", "recid": "4951", "relation": {}, "relation_version_is_last": true, "title": ["Probing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883"], "weko_shared_id": -1}
Probing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883
https://jaxa.repo.nii.ac.jp/records/4951
https://jaxa.repo.nii.ac.jp/records/495104739613-927c-45ed-a134-e17c78c84d28
名前 / ファイル | ライセンス | アクション |
---|---|---|
64574019.pdf (189.0 kB)
|
|
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Probing the Pulsar Wind in the gamma-ray Binary System: PSR B1259-63/SS 2883 | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | acceleration of particles - radiation mechanisms: non-thermal - gamma rays: theory - Xrays: binaries - pulsars: individual (PSR B1259-63) | |||||
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 |
Takata, Jumpei
× Takata, Jumpei× Taam, Ronald E. |
|||||
著者所属(英) | ||||||
en | ||||||
Department of Physics, University of Hong Kong | ||||||
著者所属(英) | ||||||
en | ||||||
Academia Sinica Institute of Astrophysics and Astronomy-TIARA | ||||||
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. 50-51, 発行日 2010-02-26 |
|||||
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 | The spectral energy distribution from the X-ray to the very high energy regime (> 100 GeV) has been investigated for the gamma-ray binary system PSR B1259-63/SS2883 as a function of orbital phase within the framework of a simple model of a pulsar wind nebula. The emission model is based on the synchrotron radiation process for the X-ray regime and the inverse Compton scattering process boosting stellar photons from the Be star companion to the very high energy (100GeV-TeV) regime. With this model, the observed temporal behavior can, in principle, be used to probe the pulsar wind properties at the shock as a function of the orbital phase. | |||||
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: AA0064574019 | |||||
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 |