{"created":"2023-07-25T08:09:29.160350+00:00","id":9099,"links":{},"metadata":{"_buckets":{"deposit":"84c1d337-a950-4332-99d1-4f9930532a10"},"_deposit":{"created_by":18,"id":"9099","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"9099"},"status":"published"},"_oai":{"id":"oai:ir.kagoshima-u.ac.jp:00009099","sets":["54:92"]},"author_link":["115028","115029","115030","115031","115032","115033","115034","115035"],"item_6_biblio_info_5":{"attribute_name":"収録雑誌名","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2012","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"5","bibliographicPageStart":"98","bibliographicVolumeNumber":"64","bibliographic_titles":[{"bibliographic_title":"Publications of the Astronomical Society of Japan","bibliographic_titleLang":"en"}]}]},"item_6_date_6":{"attribute_name":"作成日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2012-10-25","subitem_date_issued_type":"Issued"}]},"item_6_description_4":{"attribute_name":"要約(Abstract)","attribute_value_mlt":[{"subitem_description":"We observed four \"water fountain\" sources in the CO J = 3→2 line emission with the Atacama Submillimeter Telescope Experiment (ASTE) 10m telescope in 2010–2011. The water fountain sources are evolved stars that form high-velocity collimated jets traced by H2O maser emission. The CO line was detected only from IRAS 16342-3814. The present work confirmed that the 12CO to 13CO line intensity ratio is ~1.5 at the systemic velocity. We discuss the origins of the very low 12CO-to-13CO intensity ratio, as possible evidence for \"hot-bottom burning\" in an oxygen-rich star, and the CO intensity variation in IRAS 16342-3814.","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_6_publisher_23":{"attribute_name":"公開者・出版者","attribute_value_mlt":[{"subitem_publisher":"Astronomical Society of Japan","subitem_publisher_language":"en"},{"subitem_publisher":"日本天文学会","subitem_publisher_language":"ja"}]},"item_6_relation_11":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1093/pasj/64.5.98","subitem_relation_type_select":"DOI"}}]},"item_6_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"Astronomical Society of Japan","subitem_rights_language":"en"}]},"item_6_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00046264","subitem_source_identifier_type":"PISSN"}]},"item_6_source_id_9":{"attribute_name":"NII書誌ID","attribute_value_mlt":[{"subitem_source_identifier":"AA1082896X","subitem_source_identifier_type":"NCID"}]},"item_6_subject_15":{"attribute_name":"NDC","attribute_value_mlt":[{"subitem_subject":"440","subitem_subject_scheme":"NDC"}]},"item_6_version_type_14":{"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":"Imai, Hiroshi","creatorNameLang":"en"},{"creatorName":"今井, 裕","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"115028","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Chong, Sze Ning","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"115029","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"He, Jin-Hua","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"115030","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Nakashima, Jun-Ichi","creatorNameLang":"en"},{"creatorName":"中島, 淳一","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"115031","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Hsia, Chih-Hao","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"115032","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Sakai, Takeshi","creatorNameLang":"en"},{"creatorName":"酒井, 剛","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"115033","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Deguchi, Shuji","creatorNameLang":"en"},{"creatorName":"出口, 修至","creatorNameLang":"ja"}],"nameIdentifiers":[{"nameIdentifier":"115034","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Koning, Nico","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"115035","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":"2016-10-28"}],"displaytype":"detail","filename":"Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf","filesize":[{"value":"533.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf","objectType":"fulltext","url":"https://ir.kagoshima-u.ac.jp/record/9099/files/Extremely Strong 13CO J = 3→2 Line in the Water Fountain IRAS 16342-3814 Evidence for the Hot-Bottom Burning.pdf"},"version_id":"bedd815d-b9ab-4325-bcaf-d337e62514af"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"stars","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"AGB and post-AGB -- stars","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"individual (IRAS 16342-3814)","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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Extremely Strong 13CO J = 3→2 Line in the \"Water Fountain\" IRAS 16342-3814: Evidence for the Hot-Bottom Burning","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Extremely Strong 13CO J = 3→2 Line in the \"Water Fountain\" IRAS 16342-3814: Evidence for the Hot-Bottom Burning","subitem_title_language":"en"}]},"item_type_id":"6","owner":"18","path":["92"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2016-03-15"},"publish_date":"2016-03-15","publish_status":"0","recid":"9099","relation_version_is_last":true,"title":["Extremely Strong 13CO J = 3→2 Line in the \"Water Fountain\" IRAS 16342-3814: Evidence for the Hot-Bottom Burning"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2024-02-07T07:19:31.712464+00:00"}