{"created":"2023-06-19T09:12:41.977921+00:00","id":24566,"links":{},"metadata":{"_buckets":{"deposit":"7b114dc3-8119-437f-a636-3605bdc3cf4c"},"_deposit":{"created_by":12,"id":"24566","owners":[12],"pid":{"revision_id":0,"type":"depid","value":"24566"},"status":"published"},"_oai":{"id":"oai:kumadai.repo.nii.ac.jp:00024566","sets":["448:538","585:614:1055"]},"author_link":["155812","155813","155811"],"item_15_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"254","bibliographicPageStart":"247","bibliographicVolumeNumber":"13","bibliographic_titles":[{"bibliographic_title":"Physics Reports of Kumamoto University","bibliographic_titleLang":"en"}]}]},"item_15_description_5":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"Two dimensional hydrodynamical simulations of supernova remnant Cas A are performed starting from the onset of explosion to the present phase. Before the explosion, distributions of circumstellar medium is constructed, where the medium is assumed to be ejected from a progenitor. A supernova simulation is carried out by two dimensional hydrodynamical calculation. It is found that the Rayleigh-Taylor instability is advanced from the boundary between hydrogen and helium layers. The instability from silicon and iron layers is not grown enough to induce the observed mixing of materials. It is suggested that mixing before the explosion and/or instability at the boundary of silicon and iron layers due to different distributions of circumstellar medium is needed to explain the observations.","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_15_publisher_36":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"熊本大学","subitem_publisher_language":"ja"}]},"item_15_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0303-4070","subitem_source_identifier_type":"PISSN"}]},"item_15_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00774081","subitem_source_identifier_type":"NCID"}]},"item_15_subject_20":{"attribute_name":"日本十進分類法","attribute_value_mlt":[{"subitem_subject":"443.5","subitem_subject_scheme":"NDC"}]},"item_15_version_type_19":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Matsuo, Yasuhide","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155812","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hashimoto, Masa-aki","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155813","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Arai, Kenzo","creatorNameLang":"en"},{"creatorName":"荒井, 賢三","creatorNameLang":"ja"},{"creatorName":"アライ, ケンゾウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"155811","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":"2020-03-02"}],"displaytype":"detail","filename":"PR0013_247-254.pdf","filesize":[{"value":"1.5 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PR0013_247-254.pdf","url":"https://kumadai.repo.nii.ac.jp/record/24566/files/PR0013_247-254.pdf"},"version_id":"0123f0e8-23f8-4950-bd17-9aba3b87ae30"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Abundance Distribution in Supernova Remnant Cas A","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Abundance Distribution in Supernova Remnant Cas A","subitem_title_language":"en"}]},"item_type_id":"15","owner":"12","path":["538","1055"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2011-02-25"},"publish_date":"2011-02-25","publish_status":"0","recid":"24566","relation_version_is_last":true,"title":["Abundance Distribution in Supernova Remnant Cas A"],"weko_creator_id":"12","weko_shared_id":-1},"updated":"2023-10-17T06:41:12.204405+00:00"}