{"created":"2023-05-15T14:42:36.798751+00:00","id":2952,"links":{},"metadata":{"_buckets":{"deposit":"ea793fa9-13fb-4dce-8bde-3f61bc052739"},"_deposit":{"created_by":3,"id":"2952","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"2952"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:00002952","sets":["14:226:228"]},"author_link":["7890","7645"],"control_number":"2952","item_2_biblio_info_12":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2015-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"94","bibliographicPageStart":"87","bibliographicVolumeNumber":"10","bibliographic_titles":[{"bibliographic_title":"京都産業大学総合学術研究所所報"}]}]},"item_2_description_10":{"attribute_name":"抄録(日)","attribute_value_mlt":[{"subitem_description":"本稿では，遅い新星V2676 Ophに見られた，極大可視光度付近における分子生成について，神山天文台および他の天文台で行われた観測結果をもとに考察し，新星エンベロープ中における分子生成の条件について考察を行った。C₂やCN分子を作るような新星では，その分子バンド吸収スペクトルから炭素および窒素の同位体比を決定できる。こうした観測条件を満たすような新星の同定に向けた基礎的研究を行った。","subitem_description_type":"Other"}]},"item_2_description_11":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"In this study the molecular formation in classical novae is investigated, especially for the formation conditions of simple diatomic molecules like CO, CN, and C₂ in novae. From the absorption spectra of CN and C₂, it is known that the isotopic ratios of carbon and nitrogen can be obtained. Therefore, future observations of molecules in novae are important from the viewpoints of the origin of the solar system and also of the Galactic chemical evolution.","subitem_description_type":"Other"}]},"item_2_description_15":{"attribute_name":"表示順","attribute_value_mlt":[{"subitem_description":"9","subitem_description_type":"Other"}]},"item_2_description_16":{"attribute_name":"アクセション番号","attribute_value_mlt":[{"subitem_description":"KJ00009857379","subitem_description_type":"Other"}]},"item_2_description_2":{"attribute_name":"ページ属性","attribute_value_mlt":[{"subitem_description":"P","subitem_description_type":"Other"}]},"item_2_description_8":{"attribute_name":"記事種別(日)","attribute_value_mlt":[{"subitem_description":"研究活動報告","subitem_description_type":"Other"}]},"item_2_description_9":{"attribute_name":"記事種別(英)","attribute_value_mlt":[{"subitem_description":"Acitivity Reports","subitem_description_type":"Other"}]},"item_2_source_id_1":{"attribute_name":"雑誌書誌ID","attribute_value_mlt":[{"subitem_source_identifier":"AA11879037","subitem_source_identifier_type":"NCID"}]},"item_2_source_id_19":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1348-8465","subitem_source_identifier_type":"PISSN"}]},"item_2_text_6":{"attribute_name":"著者所属(日)","attribute_value_mlt":[{"subitem_text_value":"京都産業大学理学部"},{"subitem_text_value":"京都産業大学神山天文台"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"河北, 秀世","creatorNameLang":"ja"},{"creatorName":"Kawakita, Hideyo","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"新井, 彰","creatorNameLang":"ja"},{"creatorName":"Arai, Akira","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":"2018-01-28"}],"displaytype":"detail","filename":"KJ00009857379.pdf","filesize":[{"value":"416.0 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00009857379.pdf","url":"https://ksu.repo.nii.ac.jp/record/2952/files/KJ00009857379.pdf"},"version_id":"6b680d36-23c5-4455-80fd-382e6793fde2"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"古典新星","subitem_subject_scheme":"Other"},{"subitem_subject":"分子生成","subitem_subject_scheme":"Other"},{"subitem_subject":"V2676 Oph","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系起源","subitem_subject_scheme":"Other"},{"subitem_subject":"銀河系化学進化","subitem_subject_scheme":"Other"},{"subitem_subject":"Classical Novae","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Molecular formation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"V2676 Oph","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Origin of solar system","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Galactic chemical evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"jpn"}]},"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":"新星の窒素同位体比で探る太陽系起源・銀河系化学進化","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"新星の窒素同位体比で探る太陽系起源・銀河系化学進化","subitem_title_language":"ja"},{"subitem_title":"Isotopic Ratios of Carbon and Nitrogen in Novae: Clues to Origin of Solar System and Galactic Chemical Evolution","subitem_title_language":"en"}]},"item_type_id":"2","owner":"3","path":["228"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2018-01-28"},"publish_date":"2018-01-28","publish_status":"0","recid":"2952","relation_version_is_last":true,"title":["新星の窒素同位体比で探る太陽系起源・銀河系化学進化"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-09-04T05:46:36.446052+00:00"}