{"created":"2023-05-15T14:42:36.842342+00:00","id":2953,"links":{},"metadata":{"_buckets":{"deposit":"e9566b76-18ee-4a07-adec-6747ca9bad8d"},"_deposit":{"created_by":3,"id":"2953","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"2953"},"status":"published"},"_oai":{"id":"oai:ksu.repo.nii.ac.jp:00002953","sets":["14:226:228"]},"author_link":["7890","7649"],"control_number":"2953","item_2_biblio_info_12":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2015-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"100","bibliographicPageStart":"95","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，彗星氷中の窒素を含む分子について，¹⁵N濃集を調べた。彗星アンモニアにおける¹⁴N/¹⁵N ~ 150であることが我々の観測から明らかになりつつあり，この値は過去の研究で得られているCNあるいはHCNにおける値と近い。この結果から，彗星氷中のアンモニアが固体表面反応によって生成された可能性が高く，またHCNとアンモニアが共に中性窒素原子を起点とする化学反応パスによって形成された可能性を議論した。","subitem_description_type":"Other"}]},"item_2_description_11":{"attribute_name":"抄録(英)","attribute_value_mlt":[{"subitem_description":"In this study we discuss about ¹⁵N-fractionation in cometary N-bearing molecules like NH₃ and HCN. Our observations have revealed that ¹⁴N/¹⁵N ratio ~ 150 for cometary NH₂（i.e., for ammonia frozen in cometary nuclei）, which is similar to a typical value for CN and HCN. The ¹⁵N-fractionation might occur in the stage of molecular could core via grain-surface chemistry from atomic nitrogen.","subitem_description_type":"Other"}]},"item_2_description_15":{"attribute_name":"表示順","attribute_value_mlt":[{"subitem_description":"10","subitem_description_type":"Other"}]},"item_2_description_16":{"attribute_name":"アクセション番号","attribute_value_mlt":[{"subitem_description":"KJ00009857399","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":"Activity 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":"京都産業大学理学研究科"}]},"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":"新中, 善晴","creatorNameLang":"ja"},{"creatorName":"Shinnaka, Yoshiharu","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":"KJ00009857399.pdf","filesize":[{"value":"264.8 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00009857399.pdf","url":"https://ksu.repo.nii.ac.jp/record/2953/files/KJ00009857399.pdf"},"version_id":"c6eb4c3d-4649-4a0c-8d85-077ebb00ff61"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"彗星","subitem_subject_scheme":"Other"},{"subitem_subject":"分子生成","subitem_subject_scheme":"Other"},{"subitem_subject":"¹⁵N濃集","subitem_subject_scheme":"Other"},{"subitem_subject":"星間化学","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系起源","subitem_subject_scheme":"Other"},{"subitem_subject":"Comets","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Molecular formation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Fractionation of ¹⁵N","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Interstellar chemistry","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Origin of solar system","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":"近赤外線波長領域における彗星氷物質の高分散光サーベイ","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"近赤外線波長領域における彗星氷物質の高分散光サーベイ","subitem_title_language":"ja"},{"subitem_title":"High-resolution Spectroscopic Survey of Cometary Molecules in Near-infrared Wavelength Region","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":"2953","relation_version_is_last":true,"title":["近赤外線波長領域における彗星氷物質の高分散光サーベイ"],"weko_creator_id":"3","weko_shared_id":-1},"updated":"2023-09-04T05:50:18.507613+00:00"}