{"created":"2023-06-20T14:52:21.944919+00:00","id":20505,"links":{},"metadata":{"_buckets":{"deposit":"98387c78-137b-4bd2-9216-feecaadbc09e"},"_deposit":{"created_by":1,"id":"20505","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20505"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020505","sets":["1543:1778:1790","1887:1891"]},"author_link":["195851","195852","195854","195853"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-08-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"169","bibliographicPageStart":"166","bibliographic_titles":[{"bibliographic_title":"第39回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 39th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"N-body simulation to investigate the growth of embryos in a close binary system is performed. Principal targets of the simulations are to investigate the possibility of the growth of the planets from the disk of planetesimals around Alpha Centauri. The inferred stable region around the close binary system is much smaller than the Solar system. The planetesimals orbit the host star with the modulating eccentricities, but their growth proceed almost the same way in the single star because of the effect of alignment of in periastrons.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063505043","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"国立天文台"},{"subitem_text_value":"国立天文台"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"長沢, 真樹子"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小久保, 英一郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nagasawa, Makiko","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kokubo, Eiichiro","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"数値シミュレーション","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系外惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"連星","subitem_subject_scheme":"Other"},{"subitem_subject":"原始惑星系円盤","subitem_subject_scheme":"Other"},{"subitem_subject":"原始惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"ケンタウルス座アルファ星","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系","subitem_subject_scheme":"Other"},{"subitem_subject":"星周円盤","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星進化","subitem_subject_scheme":"Other"},{"subitem_subject":"脱出速度","subitem_subject_scheme":"Other"},{"subitem_subject":"地球型惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"離心率","subitem_subject_scheme":"Other"},{"subitem_subject":"numerical simulation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"extrasolar planet","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"binary star","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"protoplanetary disk","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"protoplanet","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Alpha Centauri","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar system","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"circumstellar disk","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"escape velocity","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"terrestrial planet","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"eccentricity","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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"Planetesimal growth in binary systems","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Planetesimal growth in binary systems","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1790","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20505","relation_version_is_last":true,"title":["Planetesimal growth in binary systems"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:49:20.124917+00:00"}