{"created":"2023-06-20T14:38:25.299998+00:00","id":4980,"links":{},"metadata":{"_buckets":{"deposit":"72134178-a6ce-48be-bbf9-3a9c23982e3b"},"_deposit":{"created_by":1,"id":"4980","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"4980"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00004980","sets":["1887:1891","9:789:936:948"]},"author_link":["23050","23048","23049","23052","23051","23053","23055","23054"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"125","bibliographicPageStart":"124","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 X-ray spectrum of the Galactic supernova remnant (SNR) IC 443 exhibits extremely strong radiative recombination continua (RRC). In order to study the spectrum quantitatively, we construct a semi-phenomenological model with bremsstrahlung, emission lines, and RRC. We fit the spectrum with this model and obtain reasonable agreement. By using this new model fitting, electron temperatures are obtained in three independent ways: the line flux ratios of Kbeta-Kdelta to Kalpha, the bremsstrahlung shape, and the RRC width. On the other hand, the ionization temperature is obtained by the flux ratio of H-like to He-like Kalpha lines. The fact that ionization temperature (1.1-1.4 keV) is higher than the electron temperature (0.4-1.0 keV) indicates the plasma is in an overionized state, which is very unusual for SNRs.","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: AA0064574048","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_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"京都大学大学院理学研究科物理学専攻"},{"subitem_text_value":"京都大学大学院理学研究科物理学専攻"},{"subitem_text_value":"理化学研究所"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"RIKEN (The Institute of Physical and Chemical Research)"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"小澤, 碧"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小山, 勝二"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"山口, 弘悦"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"尾崎, 正伸"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ozawa, Midori","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Koyama, Katsuji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yamaguchi, Hiroya","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ozaki, Masanobu","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"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","filename":"64574048.pdf","filesize":[{"value":"296.7 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574048.pdf","url":"https://jaxa.repo.nii.ac.jp/record/4980/files/64574048.pdf"},"version_id":"88cf462d-ecf0-4de4-8a1c-f2f27af3ddb9"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"ISM: individual (IC 443) - supernova remnants - radiation mechanisms: thermal","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":"Construction of a semi-phenomenological model for the IC 443 plasma with strong radiative recombination continua","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Construction of a semi-phenomenological model for the IC 443 plasma with strong radiative recombination continua","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["948","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"4980","relation_version_is_last":true,"title":["Construction of a semi-phenomenological model for the IC 443 plasma with strong radiative recombination continua"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:27:06.518221+00:00"}