{"created":"2023-06-20T13:22:38.242928+00:00","id":3298,"links":{},"metadata":{"_buckets":{"deposit":"e52745bf-67e7-4e0b-9389-2b31b73cdd45"},"_deposit":{"created_by":21,"id":"3298","owners":[21],"pid":{"revision_id":0,"type":"depid","value":"3298"},"status":"published"},"_oai":{"id":"oai:ir.soken.ac.jp:00003298","sets":["1:274"]},"author_link":["760","738","734"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1996-02","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicPageEnd":"17","bibliographicPageStart":"1","bibliographicVolumeNumber":"48","bibliographic_titles":[{"bibliographic_title":"Publications of the Astronomical Society of Japan  "},{"bibliographic_title":"Publications of the Astronomical Society of Japan  ","bibliographic_titleLang":"en"}]}]},"item_10001_creator_3":{"attribute_name":"著者別名","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"池内, 了"}],"nameIdentifiers":[{"nameIdentifier":"738","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"1000090025461","nameIdentifierScheme":"NRID","nameIdentifierURI":" "},{"nameIdentifier":"90025461","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=90025461"}]}]},"item_10001_description_19":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The thermal and chemical evolution of X-ray clusters of galaxies is explored, pursuing the chemical evolution and gas ejection of member galaxies. We take into account the gas-ejection processes from galaxies to intracluster space by galactic winds powered by supernovae and ram-pressure stripping. The main results are as follows:\\ \\ 1) The metal supply from elliptical galaxie s dominates over that of spirals and there is a possibility that ram pressure stripping had occurred at the same or in an earlier epoch than galactic winds i n ellipticals. \\ 2) The iron abundance of the intracluster medium (ICM) depends strongly on the initial mass function, but weakly on the star-formation rate of ellipticals, and intermediately on the wind epoch in ellipticals and the cluster richness. \\ \\ 3) The contribution to the ICM from galaxies is much smaller than that of primordial gas. ","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"The Astronomical Society of Japan"}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1093/pasj/48.1.1"}],"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"http://doi.org/10.1093/pasj/48.1.1","subitem_relation_type_select":"DOI"}}]},"item_10001_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"Copyright "}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://pasj.asj.or.jp/info/subscription.html","subitem_relation_type_select":"URI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© The Astronomical Society of Japan"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00046264","subitem_source_identifier_type":"ISSN"}]},"item_10001_version_type_20":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"FUKUMOTO, Junji"}],"nameIdentifiers":[{"nameIdentifier":"760","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"IKEUCHI, Satoru"}],"nameIdentifiers":[{"nameIdentifier":"734","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":"2014-03-10"}],"displaytype":"detail","filename":"nph-iarticle_query2.pdf","filesize":[{"value":"425.2 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"nph-iarticle_query2","url":"https://ir.soken.ac.jp/record/3298/files/nph-iarticle_query2.pdf"},"version_id":"bc2b8feb-fadd-427d-af20-a1743ee79def"}]},"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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Thermal and chemical evolution of X-ray clusters of galaxies","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Thermal and chemical evolution of X-ray clusters of galaxies"},{"subitem_title":"Thermal and chemical evolution of X-ray clusters of galaxies","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"21","path":["95","274"],"pubdate":{"attribute_name":"公開日","attribute_value":"2012-12-13"},"publish_date":"2012-12-13","publish_status":"0","recid":"3298","relation_version_is_last":true,"title":["Thermal and chemical evolution of X-ray clusters of galaxies"],"weko_creator_id":"21","weko_shared_id":21},"updated":"2023-06-20T14:33:25.261772+00:00"}