{"created":"2023-06-20T13:22:38.670891+00:00","id":3309,"links":{},"metadata":{"_buckets":{"deposit":"8591a503-ddeb-4b2c-8ce1-08de3be28a6d"},"_deposit":{"created_by":21,"id":"3309","owners":[21],"pid":{"revision_id":0,"type":"depid","value":"3309"},"status":"published"},"_oai":{"id":"oai:ir.soken.ac.jp:00003309","sets":["1:270"]},"author_link":["678","679","667","792","782","786","787","784","785","666","672","790","671","783","791","789","794","788","793","670","674"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"382","bibliographicPageStart":"375","bibliographicVolumeNumber":"58","bibliographic_titles":[{"bibliographic_title":"Publications of the Astronomical Society of Japan"},{"bibliographic_title":"Publications of the Astronomical Society of Japan","bibliographic_titleLang":"en"}]}]},"item_10001_creator_3":{"attribute_name":"著者別名","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"眞山, 聡"}],"nameIdentifiers":[{"nameIdentifier":"679","nameIdentifierScheme":"WEKO"},{"nameIdentifier":"1000020553267","nameIdentifierScheme":"NRID","nameIdentifierURI":" "},{"nameIdentifier":"20553267","nameIdentifierScheme":"e-Rad","nameIdentifierURI":"https://kaken.nii.ac.jp/ja/search/?qm=20553267"}]}]},"item_10001_description_19":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"High angular resolution near-infrared (JHK) adaptive optics images of T Tau were obtained with the infrared camera Coronagraphic Imager with Adaptive Optics (CIAO) mounted on the 8.2m Subaru Telescope in 2002 and 2004. The images resolve a complex circumstellar structure around a multiple system. We resolved T Tau Sa and Sb as well as T Tau N and S. The estimated orbit of T Tau Sb indicates that it is probably bound to T Tau Sa. The K band flux of T Tau S decreased by ˜ 1.7 Jy in 2002 November compared with that in 2001 mainly because T Tau Sa became fainter. The arc-like ridge detected in our near-infrared images is consistent with what is seen at visible wavelengths, supporting the interpretation in previous studies that the arc is part of the cavity wall seen relatively pole-on. Halo emission is detected out to ˜2''from T Tau N. This may be light scattered off the common envelope surrounding the T Tauri multiple system. ","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"The Astronomical Society of Japan"}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1093/pasj/58.2.375"}],"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1093/pasj/58.2.375","subitem_relation_type_select":"DOI"}}]},"item_10001_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"Copyright"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://pasj.asj.or.jp/info/subscription.html","subitem_relation_type_select":"URI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2006. The Astronomical Society of Japan."}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00046264","subitem_source_identifier_type":"ISSN"}]},"item_10001_version_type_20":{"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":"MAYAMA, Satoshi"}],"nameIdentifiers":[{"nameIdentifier":"666","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"TAMURA, Motohide"}],"nameIdentifiers":[{"nameIdentifier":"667","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"HAYASHI, Masahiko"},{"creatorName":"HAYASHI, Saeko S"}],"nameIdentifiers":[{"nameIdentifier":"678","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"ITOH, Yoichi"}],"nameIdentifiers":[{"nameIdentifier":"782","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"FUKAGAWA, Misato"}],"nameIdentifiers":[{"nameIdentifier":"783","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"SUTO, Hiroshi"}],"nameIdentifiers":[{"nameIdentifier":"672","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"ISHII, Miki"}],"nameIdentifiers":[{"nameIdentifier":"670","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MURAKAWA, Koji"}],"nameIdentifiers":[{"nameIdentifier":"785","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"OASA, Yumiko"}],"nameIdentifiers":[{"nameIdentifier":"784","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"YAMASHITA, Takuya"}],"nameIdentifiers":[{"nameIdentifier":"786","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MORINO, Junichi"}],"nameIdentifiers":[{"nameIdentifier":"787","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"OYA, Shin"}],"nameIdentifiers":[{"nameIdentifier":"788","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"NAOI, Takahiro"}],"nameIdentifiers":[{"nameIdentifier":"789","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"PYO, Tae-Soo"}],"nameIdentifiers":[{"nameIdentifier":"671","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"NISHIKAWA, Takayuki"}],"nameIdentifiers":[{"nameIdentifier":"790","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KUDO, Tomoyuki"}],"nameIdentifiers":[{"nameIdentifier":"674","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"USUDA, Tomonori"}],"nameIdentifiers":[{"nameIdentifier":"791","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"ANDO, Hiroyasu"}],"nameIdentifiers":[{"nameIdentifier":"792","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"MIYAMA, Shoken M"}],"nameIdentifiers":[{"nameIdentifier":"793","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"KAIFU, Norio"}],"nameIdentifiers":[{"nameIdentifier":"794","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":"2014-03-11"}],"displaytype":"simple","filename":"58022806.pdf","filesize":[{"value":"801.0 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"58022806","url":"https://ir.soken.ac.jp/record/3309/files/58022806.pdf"},"version_id":"409e0d99-dda3-40e0-bb5f-a498d7402de3"}]},"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":"Subaru near infrared coronagraphic images of T Tauri","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Subaru near infrared coronagraphic images of T Tauri"},{"subitem_title":"Subaru near infrared coronagraphic images of T Tauri","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"21","path":["152","270"],"pubdate":{"attribute_name":"公開日","attribute_value":"2012-12-20"},"publish_date":"2012-12-20","publish_status":"0","recid":"3309","relation_version_is_last":true,"title":["Subaru near infrared coronagraphic images of T Tauri"],"weko_creator_id":"21","weko_shared_id":21},"updated":"2023-06-20T14:28:13.322335+00:00"}