{"created":"2023-07-25T08:08:20.687677+00:00","id":7701,"links":{},"metadata":{"_buckets":{"deposit":"bf599226-bafe-4a23-acfe-8ba363762473"},"_deposit":{"created_by":18,"id":"7701","owners":[18],"pid":{"revision_id":0,"type":"depid","value":"7701"},"status":"published"},"_oai":{"id":"oai:ir.kagoshima-u.ac.jp:00007701","sets":["54:79"]},"author_link":["36779"],"item_8_date_6":{"attribute_name":"作成日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2011-04-22","subitem_date_issued_type":"Collected"}]},"item_8_description_4":{"attribute_name":"要約(Abstract)","attribute_value_mlt":[{"subitem_description":"2009-2010年度科学研究費補助金(研究活動スタート支援)研究成果報告書 課題番号：21840040　研究代表者：中川亜紀治 (鹿児島大学大学院理工学研究科（理学系）助教)","subitem_description_language":"ja","subitem_description_type":"Other"},{"subitem_description":"VERA電波望遠鏡を用いて高精度位置天文VLBI 観測を行ってきた。本申請課題の期間に2件の論文が日本天文学会の査読付き雑誌に掲載された。AGB星の星周現象や銀河系内での運動などが明らかになった。年周視差が計測された天体数は６天体に増え、周期光度関係確立のためのデータが揃いつつある。HIPPARCOS衛星のデータをもとにして、視線速度、距離などのデータベースを整理し、およそ300天体の銀河系内ミラ型変光星について6次元動力学情報が整理された。","subitem_description_language":"ja","subitem_description_type":"Other"},{"subitem_description":"We have conducted astrometric VLBI observations with VERA towards Galactic AGB stars. Two papers were published. In the papers, we revealed size and motion of circumstellar envelopes of two AGB stars, and tracks of a star moving in our Galaxy during recent 1Gyr. We newly detected parallaxes for 6 AGB stars and it can be used to establish more precise PLR in the Galaxy. Using the HIPPARCOS database, we compiled 6-D kinematic information for 300 AGB sources.","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_8_publisher_23":{"attribute_name":"公開者・出版者","attribute_value_mlt":[{"subitem_publisher":"鹿児島大学","subitem_publisher_language":"ja"},{"subitem_publisher":"Kagoshima University","subitem_publisher_language":"en"}]},"item_8_subject_15":{"attribute_name":"NDC","attribute_value_mlt":[{"subitem_subject":"440","subitem_subject_scheme":"NDC"}]},"item_8_text_41":{"attribute_name":"科研費番号 ","attribute_value_mlt":[{"subitem_text_value":"21840040"}]},"item_8_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":"中川, 亜紀治","creatorNameLang":"ja"},{"creatorName":"ナカガワ, アキハル","creatorNameLang":"ja-Kana"},{"creatorName":"Nakagawa, Akiharu","creatorNameLang":"en"}],"familyNames":[{},{},{}],"givenNames":[{},{},{}],"nameIdentifiers":[{"nameIdentifier":"36779","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"60535631","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=60535631"}]}]},"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":"21840040seika.pdf","filesize":[{"value":"313.9 kB"}],"format":"application/pdf","mimetype":"application/pdf","url":{"label":"21840040seika.pdf","objectType":"fulltext","url":"https://ir.kagoshima-u.ac.jp/record/7701/files/21840040seika.pdf"},"version_id":"34437ce7-86b4-4b88-87bd-c10832340dc7"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"電波天文学","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"VLBI","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"銀河系","subitem_subject_language":"ja","subitem_subject_scheme":"Other"},{"subitem_subject":"光赤外線","subitem_subject_language":"ja","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":"research report","resourceuri":"http://purl.org/coar/resource_type/c_18ws"}]},"item_title":"ミラ型変光星の精密位置天文観測による天の川銀河の動力学的研究","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"ミラ型変光星の精密位置天文観測による天の川銀河の動力学的研究","subitem_title_language":"ja"},{"subitem_title":"Kinematics of the Milky Way Galaxy using accurate astrometric observation of Mira type variables","subitem_title_language":"en"}]},"item_type_id":"8","owner":"18","path":["79"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2015-01-06"},"publish_date":"2015-01-06","publish_status":"0","recid":"7701","relation_version_is_last":true,"title":["ミラ型変光星の精密位置天文観測による天の川銀河の動力学的研究"],"weko_creator_id":"18","weko_shared_id":-1},"updated":"2024-05-23T02:18:01.438634+00:00"}