{"created":"2023-06-20T14:44:14.183784+00:00","id":11650,"links":{},"metadata":{"_buckets":{"deposit":"999dc339-d912-4683-b1d1-56fcd6cf8b82"},"_deposit":{"created_by":1,"id":"11650","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"11650"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00011650","sets":["1543:1580:1596","1887:1891"]},"author_link":["102899","102897","102898","102895","102896","102894"],"item_5_alternative_title_2":{"attribute_name":"その他のタイトル（英）","attribute_value_mlt":[{"subitem_alternative_title":"Possibility of the study of stellar mass ejection by SPICA"}]},"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2003-04","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"180","bibliographicPageStart":"177","bibliographic_titles":[{"bibliographic_title":"第3回宇宙科学シンポジウム"},{"bibliographic_title":"Proceedings of the 3rd Space Science Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_16":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"太陽などの恒星の進化の終末期は、星からの質量放出によって大きく影響される。一方、進化末期の星は、質量放出を通じて星間空間に新しく合成された元素を供給し、銀河や宇宙の進化に貢献する。これら質量放出星は赤外線で非常に明るく、赤外線天文学が始まって以来の対象である。SPICAはこのような天体についても、これまでとは質的に異なる情報をもたらし、研究を大きく進める可能性を持つ。SPICAに期待される進化末期天体の観測と、それによって得られるであろう成果について議論する。","subitem_description_type":"Abstract"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0045441045","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙科学研究所"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"The Institute of Space and Astronautical Science (ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"宇宙科学研究所"},{"subitem_text_value":"国立天文台 岡山観測所"},{"subitem_text_value":"東京大学 大学院理学系研究科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Institute of Space and Astronautical Science"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory Okayama Astrophysical Observatory"},{"subitem_text_language":"en","subitem_text_value":"University of Tokyo Graduate School of Science"}]},"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":"山村, 一誠"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"泉浦, 秀行"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松永, 典之"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yamamura, Issei","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Izumiura, Hideyuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsunaga, Noriyuki","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"恒星大気","subitem_subject_scheme":"Other"},{"subitem_subject":"SPICAミッション","subitem_subject_scheme":"Other"},{"subitem_subject":"赤外望遠鏡","subitem_subject_scheme":"Other"},{"subitem_subject":"宇宙論","subitem_subject_scheme":"Other"},{"subitem_subject":"天体物理学","subitem_subject_scheme":"Other"},{"subitem_subject":"質量放出","subitem_subject_scheme":"Other"},{"subitem_subject":"銀河系進化","subitem_subject_scheme":"Other"},{"subitem_subject":"星生成","subitem_subject_scheme":"Other"},{"subitem_subject":"高位置分解能","subitem_subject_scheme":"Other"},{"subitem_subject":"研究開発","subitem_subject_scheme":"Other"},{"subitem_subject":"star atmosphere","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"SPICA mission","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"infrared telescope","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"cosmology","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"astrophysics","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"mass ejection","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"galactic evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"star formation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"high spatial resolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"research and development","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":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"SPICAによる質量放出星研究の可能性","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"SPICAによる質量放出星研究の可能性"}]},"item_type_id":"5","owner":"1","path":["1596","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"11650","relation_version_is_last":true,"title":["SPICAによる質量放出星研究の可能性"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T06:34:06.234850+00:00"}