{"created":"2023-06-20T14:36:40.520390+00:00","id":3023,"links":{},"metadata":{"_buckets":{"deposit":"633d789b-1bc8-4e4a-a130-4e6a1c9a2474"},"_deposit":{"created_by":1,"id":"3023","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"3023"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00003023","sets":["1887:1891","9:789:806:807"]},"author_link":["10586","10587","10589","10585","10590","10584","10591","10588"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2018-03-09","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"218","bibliographicPageStart":"215","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's 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's 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":"Polycyclic aromatic hydrocarbons (PAHs) are some of the important components of the interstellar medium being both abundant and ubiquitous. We present the preliminary results on PAH emission in HII regions in the Large Magellanic Cloud using the spectroscopic data taken by Infrared Spectrograph (IRS; 5-38 μm), a part of the SAGE-Spec Spitzer Legacy program. The SAGE-Spec program provides the IRS mapping data of ten HII regions combining them with the archival data of 30 Dor. Among the eleven HII regions, an exemplary spectrum of an HII region (LHA 120-N 11: DEM L34) is presented. The integrated spectrum shows prominent PAH features at 6.2, 7 to 9, and 11.3 μm as well as a weak PAH feature at 12.7 μm. Several ionic lines such as [S IV] 10.51, [Ne II] 12. 81, and [Ne III] 15.56 μm, are also detected, which probe the ionization and/or density of the gas. PAH band ratios are examined over the region, and we investigate the correlation between the band ratios and the radiation field strength. Finally, we propose how the nature of PAHs and their correlation to the local environment can be extensively explored by SPICA.","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: AA1730027046","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_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan"},{"subitem_text_language":"en","subitem_text_value":"Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan"},{"subitem_text_language":"en","subitem_text_value":"Max Planck Institute for Astronomy"},{"subitem_text_language":"en","subitem_text_value":"CEA Saclay"},{"subitem_text_language":"en","subitem_text_value":"CEA Saclay"},{"subitem_text_language":"en","subitem_text_value":"Space Telescope Science Institute (STScI)"},{"subitem_text_language":"en","subitem_text_value":"University of Virginia"},{"subitem_text_language":"en","subitem_text_value":"CEA Saclay"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Seok, Ji-Yeon","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kemper, Francisca","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Hony, Sacha","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Madden, Suzanne","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Galliano, Frederic","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Gordon, Karl","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Indebetouw, Remy","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Lebouteiller, Vianney","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"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","filename":"AA1730027046.pdf","filesize":[{"value":"749.6 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AA1730027046.pdf","url":"https://jaxa.repo.nii.ac.jp/record/3023/files/AA1730027046.pdf"},"version_id":"a183cf6f-7c27-430e-9f44-08cc1448226d"}]},"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":"PAH Emission from HII Regions in the SAGE-spec Spitzer Program","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"PAH Emission from HII Regions in the SAGE-spec Spitzer Program","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["807","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2018-05-01"},"publish_date":"2018-05-01","publish_status":"0","recid":"3023","relation_version_is_last":true,"title":["PAH Emission from HII Regions in the SAGE-spec Spitzer Program"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T09:11:45.918404+00:00"}