{"created":"2023-06-20T15:07:17.875630+00:00","id":36657,"links":{},"metadata":{"_buckets":{"deposit":"ef74ee3a-4d55-4ce6-835f-4c1d52d964e7"},"_deposit":{"created_by":1,"id":"36657","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"36657"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00036657","sets":["1887:1890","1896:1898:1899:1991"]},"author_link":["424150","424151","424153","424152"],"item_9_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2000-12","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"57","bibliographicPageStart":"51","bibliographicVolumeNumber":"14","bibliographic_titles":[{},{"bibliographic_title":"The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission","bibliographic_titleLang":"en"}]}]},"item_9_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We present a brief summary of the ISO survey of AGB stars in 8 populous intermediateage clusters of the Magellanic Clouds. Totally, more than 100 AGB and RGB stars were observed at 4.5, 6.7 and 12 μm. We introduce a new method to estimate effective temperatures of oxygen-rich AGB stars, and derive precise Mbol and Teff for a large population of AGB objects in both LMC and SMC. The derived stellar parameters are used to construct observed HR diagrams whichare employed further to estimate cluster ages using the isochrone fitting. We show that proposed method gives a powerful tool to study AGB star populations within the Local Group galaxies, especially, when backed up with the observations from forthcoming mid-IR astronomical spacefacilities (ASTRO-F, SIRTF) and large ground-based telescopes (SUBARU, VLT, etc.).","subitem_description_type":"Other"}]},"item_9_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: SA4586412000","subitem_description_type":"Other"}]},"item_9_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙科学研究所"}]},"item_9_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science"}]},"item_9_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0288-433X","subitem_source_identifier_type":"ISSN"}]},"item_9_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA10455137","subitem_source_identifier_type":"NCID"}]},"item_9_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":"Institute of Physics"},{"subitem_text_language":"en","subitem_text_value":"CEA.DSM.DAPNIA.Service of d'Astrophys"},{"subitem_text_language":"en","subitem_text_value":"Institute of Astronomy, School of Science, The University of Tokyo"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Arunas, KU&#268 INSKAS","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"424150","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Vladas, VANSEVI&#268 IUS","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"424151","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Marc, SAUVAGE","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"424152","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Toshihiko, TANAB&Eacute","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"424153","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":"2020-01-24"}],"displaytype":"detail","filename":"SA4586412.pdf","filesize":[{"value":"222.4 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"SA4586412.pdf","url":"https://jaxa.repo.nii.ac.jp/record/36657/files/SA4586412.pdf"},"version_id":"95b717e2-6d5d-4106-9669-cc6a28f361d0"}]},"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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Mid-infrared Studies of the AGB Star Populations in the Local Group Galaxies : the Magellanic Clouds","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Mid-infrared Studies of the AGB Star Populations in the Local Group Galaxies : the Magellanic Clouds","subitem_title_language":"en"}]},"item_type_id":"9","owner":"1","path":["1890","1991"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"36657","relation_version_is_last":true,"title":["Mid-infrared Studies of the AGB Star Populations in the Local Group Galaxies : the Magellanic Clouds"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T22:51:55.800894+00:00"}