{"created":"2023-06-20T14:38:26.673354+00:00","id":5003,"links":{},"metadata":{"_buckets":{"deposit":"4732afa1-9b05-4455-be51-421cddf68506"},"_deposit":{"created_by":1,"id":"5003","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5003"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005003","sets":["1887:1891","9:789:936:948"]},"author_link":["23254","23251","23259","23257","23255","23260","23252","23250","23248","23253","23256","23258","23249"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"199","bibliographicPageStart":"198","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":"We report on preliminary results of the Suzaku observations of the W-R binary WR 140 (WC7+O5I), with the aim of understanding the W-R stellar wind as well as the wind-wind collision shocks. Our observations with exposures of 210 ksec in total were made at four different epochs around periastron passage in Jan. 2009. We detected hard X-ray excess in the HXD band. This is the first time that the hard X-ray excess above 10 keV was detected from a W-R binary. Moreover, we found a part of the soft component is not absorbed even by the dense wind. The spectra can be fitted by three different components, with a stationary soft component at kT approximately 0.1 keV, a high temperature component at kT approximately 3 keV and a harder power-low component. The column density at periastron is a factor of 30 higher than that at pre-periastron, which can be explained as self-absorption of the W-R wind. It is found that the emission measure of high temperature component is not proportional to the inverse of the separation of the two stars.","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: AA0064574071","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":"中央大学理工学部物理学科"},{"subitem_text_value":"宇宙航空研究開発機構宇宙科学研究本部"},{"subitem_text_value":"中央大学理工学部物理学科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Faculty of Science & Engineering, Chuo University"},{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS)(JAXA)"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Faculty of Science & Engineering, Chuo University"},{"subitem_text_language":"en","subitem_text_value":"CRESST and X-ray Astrophysics Laboratory NASA/GSFC"},{"subitem_text_language":"en","subitem_text_value":"CRESST and X-ray Astrophysics Laboratory NASA/GSFC"},{"subitem_text_language":"en","subitem_text_value":"European Space Agency, XMM-Newton Science Operations Centre, European Space Astronomy Centre"},{"subitem_text_language":"en","subitem_text_value":"Departement de Physique, Universite de Montreal"},{"subitem_text_language":"en","subitem_text_value":"Institute for Astronomy, Royal Observatory"},{"subitem_text_language":"en","subitem_text_value":"National Research Council of Canada"},{"subitem_text_language":"en","subitem_text_value":"School of Physics and Astronomy, The University of Leeds"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"菅原, 泰晴"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"前田, 良知"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"坪井, 陽子"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Sugawara, Yasuharu","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Maeda, Yoshitomo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tsuboi, Yohko","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hamaguchi, Kenji","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Corcoran, Michael","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Pollock, Andy","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Moffat, Anthony","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Williams, Peredur","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Dougherty, Sean","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Pittard, Julian","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":"64574071.pdf","filesize":[{"value":"374.3 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574071.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5003/files/64574071.pdf"},"version_id":"23941069-7a04-4bc3-8730-6995f77898a9"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"stars: Wolf-Rayet - binaries: spectroscopic - stars: WR140","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":"X-ray monitoring of the Wolf-Rayet binary WR140 with Suzaku","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"X-ray monitoring of the Wolf-Rayet binary WR140 with Suzaku","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":"5003","relation_version_is_last":true,"title":["X-ray monitoring of the Wolf-Rayet binary WR140 with Suzaku"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:26:24.706019+00:00"}