{"created":"2023-07-27T04:39:28.697917+00:00","id":12120,"links":{},"metadata":{"_buckets":{"deposit":"133c6dba-caab-4214-b189-27f430a7a6cd"},"_deposit":{"created_by":3,"id":"12120","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"12120"},"status":"published"},"_oai":{"id":"oai:tohoku.repo.nii.ac.jp:00012120","sets":["91:156"]},"author_link":["26725"],"item_4_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1981-12-05","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"3","bibliographicPageEnd":"142","bibliographicPageStart":"130","bibliographicVolumeNumber":"2","bibliographic_titles":[{"bibliographic_title":"The science reports of the Tohoku University. Ser. 8, Physics and astronomy"}]}]},"item_4_date_62":{"attribute_name":"登録日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-05-02","subitem_date_issued_type":"Created"}]},"item_4_date_63":{"attribute_name":"公開日（投稿完了日）","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-05-02","subitem_date_issued_type":"Created"}]},"item_4_date_65":{"attribute_name":"発行日","attribute_value_mlt":[{"subitem_date_issued_datetime":"1981-12-05","subitem_date_issued_type":"Created"}]},"item_4_date_80":{"attribute_name":"更新日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2010-01-27","subitem_date_issued_type":"Created"}]},"item_4_description_15":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_4_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The circumstellar gas of helium-rich stars will be trapped in the outer region of stellar magnetosphere where the centrifugal force dominates. Only in rapidly rotating stars, the outer region can contain the gas much enough to emit the observed Hα emission energy flux. As the circumstellar gas corotates with the star, the Hα emission profile becomes very broad and so the emission will appear in the wing of Hα absorption line which originates in the photosphere of star.","subitem_description_type":"Abstract"}]},"item_4_description_41":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"subitem_description":"紀要類(bulletin)","subitem_description_type":"Other"}]},"item_4_description_66":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"563203 bytes","subitem_description_type":"Other"}]},"item_4_publisher_34":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Faculty of Science, Tohoku University"}]},"item_4_radio_69":{"attribute_name":"公開範囲","attribute_value_mlt":[{"subitem_radio_item":"学外"}]},"item_4_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"03885607","subitem_source_identifier_type":"ISSN"}]},"item_4_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00441828","subitem_source_identifier_type":"NCID"}]},"item_4_version_type_16":{"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":"NAKAJIMA, Ryuzo"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2017-02-03"}],"displaytype":"detail","filename":"KJ00004424186.pdf","filesize":[{"value":"563.2 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00004424186.pdf","url":"https://tohoku.repo.nii.ac.jp/record/12120/files/KJ00004424186.pdf"},"version_id":"db66a7f2-4482-4175-9017-0957a1538565"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Helium-rich stars","subitem_subject_scheme":"Other"},{"subitem_subject":"Hα emission","subitem_subject_scheme":"Other"},{"subitem_subject":"Stellar Magnetosphere","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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"The Hα Emission of Helium-rich Stars","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The Hα Emission of Helium-rich Stars"}]},"item_type_id":"4","owner":"3","path":["156"],"pubdate":{"attribute_name":"公開日","attribute_value":"2008-05-02"},"publish_date":"2008-05-02","publish_status":"0","recid":"12120","relation_version_is_last":true,"title":["The Hα Emission of Helium-rich Stars"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2023-07-27T16:17:04.610872+00:00"}