{"created":"2023-06-20T14:43:20.884244+00:00","id":10677,"links":{},"metadata":{"_buckets":{"deposit":"9423f945-09f9-4100-83e7-ef10ec303b72"},"_deposit":{"created_by":1,"id":"10677","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"10677"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00010677","sets":["1543:1580:1589","1887:1891"]},"author_link":["89971","89964","89966","89974","89969","89975","89970","89972","89965","89967","89973","89976","89968","89977"],"item_5_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Determination of heavy elemental composition in the high temperature-interstellar medium of the early type galaxies by Suzaku satellite"}]},"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-01","bibliographicIssueDateType":"Issued"},"bibliographicVolumeNumber":"10","bibliographic_titles":[{"bibliographic_title":"宇宙科学シンポジウム: 講演集録"},{"bibliographic_title":"Proceedings of the Space Science Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_14":{"attribute_name":"会議概要（会議名, 開催地, 会期, 主催者等）","attribute_value_mlt":[{"subitem_description":"第10回宇宙科学シンポジウム (2010年1月7日-8日. 宇宙航空研究開発機構宇宙科学研究本部)","subitem_description_type":"Other"}]},"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":"10th Space Science Symposium (January 7-8, 2010. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan","subitem_description_type":"Other"}]},"item_5_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"すざく衛星の優れたエネルギー分解能を用いることにより、４つの楕円銀河と2つのS0銀河の高温星間ガスの重元素組成を調べることができた。早期型銀河では、晩期型星からの質量放出により高温ガスが供給され、Ia型超新星爆発によって汚染される。観測された高温ガスの鉄の組成が太陽と同程度であったことは、現在のIa型超新星爆発率は低いことを示唆する。酸素、ネオン、マグネシウム、ケイ素、硫黄、鉄の組成比も太陽と同程度であった。Ia型超新星爆発による汚染を考えると、早期型銀河の星の組成は太陽よりもII型超新星からの寄与を多く含むことなる。これは早期型銀河では星形成の時間スケールが短かったことを示唆する。","subitem_description_type":"Abstract"}]},"item_5_description_18":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"形態: カラー図版あり","subitem_description_type":"Other"},{"subitem_description":"形態: CD-ROM1枚","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Physical characteristics: Original contains color illustrations","subitem_description_type":"Other"},{"subitem_description":"Note: One CD-ROM","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064742186","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)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"東京理科大学"},{"subitem_text_value":"東京理科大学"},{"subitem_text_value":"東京理科大学"},{"subitem_text_value":"東京理科大学"},{"subitem_text_value":"広島大学"},{"subitem_text_value":"広島大学"},{"subitem_text_value":"名古屋大学"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Tokyo University of Science"},{"subitem_text_language":"en","subitem_text_value":"Tokyo University of Science"},{"subitem_text_language":"en","subitem_text_value":"Tokyo University of Science"},{"subitem_text_language":"en","subitem_text_value":"Tokyo University of Science"},{"subitem_text_language":"en","subitem_text_value":"Hiroshima University"},{"subitem_text_language":"en","subitem_text_value":"Hiroshima University"},{"subitem_text_language":"en","subitem_text_value":"Nagoya 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":"松下, 恭子"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"薙野, 綾"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小波, さおり"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"戸塚, 都"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"深沢, 泰司"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"林, 克洋"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"田原, 譲"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsushita, Kyoko","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nagino, Ryo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Konami, Saori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tozuka, Miyako","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Fukazawa, Yasushi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hayashi, Katsuhiro","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tawara, Yuzuru","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"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":"すざく衛星による早期型銀河の高温星間ガスの重元素組成の決定","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"すざく衛星による早期型銀河の高温星間ガスの重元素組成の決定"}]},"item_type_id":"5","owner":"1","path":["1589","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"10677","relation_version_is_last":true,"title":["すざく衛星による早期型銀河の高温星間ガスの重元素組成の決定"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T06:48:29.752574+00:00"}