WEKO3
アイテム
{"_buckets": {"deposit": "b719e3dd-da72-431b-a5cf-d186ea49d961"}, "_deposit": {"created_by": 1, "id": "3041", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "3041"}, "status": "published"}, "_oai": {"id": "oai:jaxa.repo.nii.ac.jp:00003041", "sets": ["807", "1891"]}, "author_link": ["10764", "10765", "10763", "10759", "10760", "10761", "10766", "10762"], "item_5_biblio_info_10": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2018-03-09", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "296", "bibliographicPageStart": "293", "bibliographicVolumeNumber": "JAXA-SP-17-010E", "bibliographic_titles": [{"bibliographic_title": "宇宙航空研究開発機構特別資料"}, {"bibliographic_title": "JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA\u0027s New Window on the Cool Universe", "bibliographic_titleLang": "en"}]}]}, "item_5_description_15": {"attribute_name": "会議概要(会議名, 開催地, 会期, 主催者等)(英)", "attribute_value_mlt": [{"subitem_description": "SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA\u0027s New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan", "subitem_description_type": "Other"}]}, "item_5_description_17": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "We built up a new observation system for investigation of massive star clusters. The tool is NIR imaging photometry by broad- and narrow-band filters installed in Atacama Near-InfraRed camera (ANIR). The observations of massive star clusters were carried out with mini-TAO 1m telescope. As the results, almost all of known Wolf-Rayet (WR) stars or luminous-blue variables (LBVs) were confined and new candidates of progenitors of supernovae (SNe) were detected. Color-color diagram (brackets N207/Ks brackets vs brackets N187/Ks brackets) made from the images clearly shows a zone of 1.87 micrometers excess due to He II and Paschen-alpha emission that indicates WN-type WR stars and LBVs, and a zone of 2.07 micrometers excess due to C IV emission from WC-type WR stars. In other words, we found that various types of massive stars can be classified as zones on the diagram. Furthermore we will be able to reveal not only buried WR stars but also the constituent, age and evolution of massive star clusters. Identification of the components of clusters with mini-TAO, TAO 6.5m and SPICA gives significant information to clarify the history of star formation (the birth and the evolution) of massive star clusters.", "subitem_description_type": "Other"}]}, "item_5_description_18": {"attribute_name": "内容記述", "attribute_value_mlt": [{"subitem_description": "形態: カラー図版あり", "subitem_description_type": "Other"}]}, "item_5_description_19": {"attribute_name": "内容記述(英)", "attribute_value_mlt": [{"subitem_description": "Physical characteristics: Original contains color illustrations", "subitem_description_type": "Other"}]}, "item_5_description_32": {"attribute_name": "資料番号", "attribute_value_mlt": [{"subitem_description": "資料番号: AA1730027064", "subitem_description_type": "Other"}]}, "item_5_description_33": {"attribute_name": "レポート番号", "attribute_value_mlt": [{"subitem_description": "レポート番号: JAXA-SP-17-010E", "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(JAXA)"}]}, "item_5_publisher_9": {"attribute_name": "出版者(英)", "attribute_value_mlt": [{"subitem_publisher": "Japan Aerospace Exploration Agency (JAXA)"}]}, "item_5_source_id_22": {"attribute_name": "ISSNONLINE", "attribute_value_mlt": [{"subitem_source_identifier": "2433-2232", "subitem_source_identifier_type": "ISSN"}]}, "item_5_text_34": {"attribute_name": "メタデータ提供者", "attribute_value_mlt": [{"subitem_text_value": "メタデータ提供者: JAXA"}]}, "item_5_text_35": {"attribute_name": "JAXAカテゴリ", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ: 特別資料"}]}, "item_5_text_36": {"attribute_name": "JAXAカテゴリ2", "attribute_value_mlt": [{"subitem_text_value": "JAXAカテゴリ2: IS"}]}, "item_5_text_38": {"attribute_name": "NASA分類コード", "attribute_value_mlt": [{"subitem_text_value": "NASA分類コード: 89"}]}, "item_5_text_39": {"attribute_name": "NASA分類表目標", "attribute_value_mlt": [{"subitem_text_value": "NASA分類: Astronomy"}]}, "item_5_text_40": {"attribute_name": "jaxa出版物種類", "attribute_value_mlt": [{"subitem_text_value": "jaxa出版物種類: SP"}]}, "item_5_text_43": {"attribute_name": "DSpaceコレクション番号", "attribute_value_mlt": [{"subitem_text_value": "DSpaceコレクション番号: 10"}]}, "item_5_text_6": {"attribute_name": "著者所属", "attribute_value_mlt": [{"subitem_text_value": "東京大学"}, {"subitem_text_value": "東京大学"}, {"subitem_text_value": "日本スペースガード協会"}]}, "item_5_text_7": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "The University of Tokyo"}, {"subitem_text_language": "en", "subitem_text_value": "The University of Tokyo"}, {"subitem_text_language": "en", "subitem_text_value": "Japan Spaceguard Association"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "高橋, 英則"}], "nameIdentifiers": [{"nameIdentifier": "10759", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "田中, 培生"}], "nameIdentifiers": [{"nameIdentifier": "10760", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "奥村, 真一郎"}], "nameIdentifiers": [{"nameIdentifier": "10761", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "TAO team"}], "nameIdentifiers": [{"nameIdentifier": "10762", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Takahashi, Hidenori", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "10763", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Tanaka, Masuo", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "10764", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Okumura, Shinichiro", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "10765", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "TAO team", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "10766", "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": "2020-01-15"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "AA1730027064.pdf", "filesize": [{"value": "1.5 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1500000.0, "url": {"label": "AA1730027064.pdf", "url": "https://jaxa.repo.nii.ac.jp/record/3041/files/AA1730027064.pdf"}, "version_id": "718f88d8-361d-4b9c-b1a1-fad074fa2990"}]}, "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": "Investigation of Property of Massive Star Clusters by mini-TAO, TAO and SPICA", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Investigation of Property of Massive Star Clusters by mini-TAO, TAO and SPICA", "subitem_title_language": "en"}]}, "item_type_id": "5", "owner": "1", "path": ["807", "1891"], "permalink_uri": "https://jaxa.repo.nii.ac.jp/records/3041", "pubdate": {"attribute_name": "公開日", "attribute_value": "2018-05-01"}, "publish_date": "2018-05-01", "publish_status": "0", "recid": "3041", "relation": {}, "relation_version_is_last": true, "title": ["Investigation of Property of Massive Star Clusters by mini-TAO, TAO and SPICA"], "weko_shared_id": 1}
Investigation of Property of Massive Star Clusters by mini-TAO, TAO and SPICA
https://jaxa.repo.nii.ac.jp/records/3041
https://jaxa.repo.nii.ac.jp/records/304112a008c7-93f6-4276-a373-00ac13f76f28
名前 / ファイル | ライセンス | アクション |
---|---|---|
AA1730027064.pdf (1.5 MB)
|
|
Item type | 会議発表論文 / Conference Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 2018-05-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Investigation of Property of Massive Star Clusters by mini-TAO, TAO and SPICA | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||
資源タイプ | conference paper | |||||
著者 |
高橋, 英則
× 高橋, 英則× 田中, 培生× 奥村, 真一郎× TAO team× Takahashi, Hidenori× Tanaka, Masuo× Okumura, Shinichiro× TAO team |
|||||
著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
日本スペースガード協会 | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
Japan Spaceguard Association | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構(JAXA) | |||||
出版者(英) | ||||||
出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||
書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe 巻 JAXA-SP-17-010E, p. 293-296, 発行日 2018-03-09 |
|||||
会議概要(会議名, 開催地, 会期, 主催者等)(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We built up a new observation system for investigation of massive star clusters. The tool is NIR imaging photometry by broad- and narrow-band filters installed in Atacama Near-InfraRed camera (ANIR). The observations of massive star clusters were carried out with mini-TAO 1m telescope. As the results, almost all of known Wolf-Rayet (WR) stars or luminous-blue variables (LBVs) were confined and new candidates of progenitors of supernovae (SNe) were detected. Color-color diagram (brackets N207/Ks brackets vs brackets N187/Ks brackets) made from the images clearly shows a zone of 1.87 micrometers excess due to He II and Paschen-alpha emission that indicates WN-type WR stars and LBVs, and a zone of 2.07 micrometers excess due to C IV emission from WC-type WR stars. In other words, we found that various types of massive stars can be classified as zones on the diagram. Furthermore we will be able to reveal not only buried WR stars but also the constituent, age and evolution of massive star clusters. Identification of the components of clusters with mini-TAO, TAO 6.5m and SPICA gives significant information to clarify the history of star formation (the birth and the evolution) of massive star clusters. | |||||
内容記述 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 形態: カラー図版あり | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Physical characteristics: Original contains color illustrations | |||||
ISSNONLINE | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 2433-2232 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA1730027064 | |||||
レポート番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | レポート番号: JAXA-SP-17-010E |