{"created":"2023-06-20T14:43:53.510259+00:00","id":11259,"links":{},"metadata":{"_buckets":{"deposit":"a7e00e06-33e2-4fa2-af3b-569c6ea812ba"},"_deposit":{"created_by":1,"id":"11259","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"11259"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00011259","sets":["1543:1580:1594","1887:1891"]},"author_link":["98652","98651","98655","98653","98654","98648","98649","98650"],"item_5_alternative_title_2":{"attribute_name":"その他のタイトル(英)","attribute_value_mlt":[{"subitem_alternative_title":"High energy phenomena in the center of Milky Way Galaxy studied by NeXT"}]},"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2005-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"19","bibliographicPageStart":"16","bibliographic_titles":[{"bibliographic_title":"第5回宇宙科学シンポジウム"},{"bibliographic_title":"Proceedings of the 5th Space Science Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Astro-E2の次のX線天文衛星として計画が進められているNeXT衛星は、10keVを越える硬X線領域での撮像分光観測を目標としている。特に様々な高エネルギー現象が集中している我々の銀河系の中心領域では大きな成果を挙げることが期待される。本稿ではその主なものとして、(1)最高エネルギー粒子の探索による宇宙線の加速源の特定、(2)X線反射星雲による巨大ブラックホールの活動履歴の解明、(3)Ti-44からの輝線によるごく最近の超新星爆発レートの決定、について紹介する。","subitem_description_type":"Abstract"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0049122005","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宇宙科学研究本部"}]},"item_5_publisher_9":{"attribute_name":"出版者(英)","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"宇宙航空研究開発機構 宇宙科学研究本部"},{"subitem_text_value":"宇宙航空研究開発機構 宇宙科学研究本部"},{"subitem_text_value":"京都大学"},{"subitem_text_value":"京都大学"}]},"item_5_text_7":{"attribute_name":"著者所属(英)","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Japan Aerospace Exploration Agency Institute of Space and Astronautical Science"},{"subitem_text_language":"en","subitem_text_value":"Japan Aerospace Exploration Agency Institute of Space and Astronautical Science"},{"subitem_text_language":"en","subitem_text_value":"Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Kyoto University"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"村上, 弘志"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"前田, 良知"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小山, 勝二"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"千田, 篤史"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Murakami, Hiroshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Maeda, Yoshitomo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Koyama, Katsuji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Senda, Atsushi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"NeXT","subitem_subject_scheme":"Other"},{"subitem_subject":"銀河","subitem_subject_scheme":"Other"},{"subitem_subject":"シンクロトロン放射","subitem_subject_scheme":"Other"},{"subitem_subject":"天文衛星","subitem_subject_scheme":"Other"},{"subitem_subject":"ブラックホール","subitem_subject_scheme":"Other"},{"subitem_subject":"星雲","subitem_subject_scheme":"Other"},{"subitem_subject":"超新星","subitem_subject_scheme":"Other"},{"subitem_subject":"分子雲","subitem_subject_scheme":"Other"},{"subitem_subject":"最高エネルギー粒子","subitem_subject_scheme":"Other"},{"subitem_subject":"硬X線撮像","subitem_subject_scheme":"Other"},{"subitem_subject":"X線スペクトロスコピー","subitem_subject_scheme":"Other"},{"subitem_subject":"宇宙線","subitem_subject_scheme":"Other"},{"subitem_subject":"非熱的フィラメント","subitem_subject_scheme":"Other"},{"subitem_subject":"NeXT","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"galaxy","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"synchrotron radiation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"astronomical satellite","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"black hole","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"nebula","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"supernova","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"molecular cloud","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"highest energy particle","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"hard X-ray imagery","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"X-ray spectroscopy","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"cosmic ray","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"non-thermal filament","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"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":"NeXTで探る我々の銀河系中心部の高エネルギー現象","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"NeXTで探る我々の銀河系中心部の高エネルギー現象"}]},"item_type_id":"5","owner":"1","path":["1594","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"11259","relation_version_is_last":true,"title":["NeXTで探る我々の銀河系中心部の高エネルギー現象"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T06:40:04.091519+00:00"}