{"created":"2023-06-20T14:38:28.682041+00:00","id":5048,"links":{},"metadata":{"_buckets":{"deposit":"cd38b483-a642-43e4-8eed-c89201feed4e"},"_deposit":{"created_by":1,"id":"5048","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"5048"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00005048","sets":["1887:1891","9:789:936:948"]},"author_link":["23619","23622","23616","23613","23623","23615","23617","23614","23618","23620","23621"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010-02-26","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"307","bibliographicPageStart":"306","bibliographicVolumeNumber":"JAXA-SP-09-008E","bibliographic_titles":[{"bibliographic_title":"宇宙航空研究開発機構特別資料:"},{"bibliographic_title":"JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H","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":"The 3rd Suzaku international Conference \"Energetic Cosmos : from Suzaku to ASTRO-H\" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan","subitem_description_type":"Other"}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Supercritical accretion flows inevitably produce radiation-pressure driven outflows, which will Compton up-scatter soft photons from the underlying accretion flow, thereby making hard emission. We performed two dimensional radiation hydrodynamic simulations of supercritical accretion flows and outflows, incorporating such Compton scattering effects, and demonstrate that there appears a new hard spectral state \"Comptonizing outflow state\" at higher photon luminosities than that of the slim-disk state. In this state, as the photon luminosity increases, the photon index decreases and the fraction of the hard emission increases. The Compton y-parameter is of the order of unity (and thus the photon index will be approximately 2) when the apparent photon luminosity is approximately 30L(sub　E) (with L(sub E) being the Eddington luminosity) for nearly face-on sources. This explains the fact that brighter ULXs possess harder X-ray spectra (Berghea et al. 2008). Furthermore, expected SED of the Comptonizing outflow state is consistent with that of the ultraluminous state, which consists of the disk and the cool, optically thick corona (Gladstone et al. 2009).","subitem_description_type":"Other"}]},"item_5_description_19":{"attribute_name":"内容記述（英）","attribute_value_mlt":[{"subitem_description":"Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0064574116","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-09-008E","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"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Japan Aerospace Exploration Agency (JAXA)"}]},"item_5_source_id_21":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"1349-113X","subitem_source_identifier_type":"ISSN"}]},"item_5_source_id_24":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA11984031","subitem_source_identifier_type":"NCID"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"千葉大学理学研究科物理学コース"},{"subitem_text_value":"国立天文台"},{"subitem_text_value":"京都大学大学院理学研究科宇宙物理学教室"},{"subitem_text_value":"京都大学大学院理学研究科宇宙物理学教室"},{"subitem_text_value":"大阪大学レーザーエネルギー学研究センター"},{"subitem_text_value":"千葉大学理学研究科物理学コース"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Graduate School of Science, Chiba University"},{"subitem_text_language":"en","subitem_text_value":"National Astronomical Observatory of Japan"},{"subitem_text_language":"en","subitem_text_value":"Department of Astronomy, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Department of Astronomy, Kyoto University"},{"subitem_text_language":"en","subitem_text_value":"Institute of Laser Engineering, Osaka University"},{"subitem_text_language":"en","subitem_text_value":"Department of Physics, Graduate School of Science, Chiba University"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"川島, 朋尚"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"大須賀, 健"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"嶺重, 慎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"高部, 英明"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"松元, 亮治"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kawashima, Tomohisa","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Ohsuga, Ken","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Mineshige, Shin","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Heinzeller, Dominikus","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Takabe, Hideaki","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Matsumoto, Ryoji","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":"2020-01-16"}],"displaytype":"detail","filename":"64574116.pdf","filesize":[{"value":"179.1 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"64574116.pdf","url":"https://jaxa.repo.nii.ac.jp/record/5048/files/64574116.pdf"},"version_id":"738bbc2b-f69e-4189-bf57-6641609745d0"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"accretion, accretion disks - black hole physics - hydrodynamics - radiative transfer","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"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":"New Spectral State of Supercritical Accretion Flow with Comptonizing Outflow:  Application to Bright ULXs","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"New Spectral State of Supercritical Accretion Flow with Comptonizing Outflow:  Application to Bright ULXs","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["948","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"5048","relation_version_is_last":true,"title":["New Spectral State of Supercritical Accretion Flow with Comptonizing Outflow:  Application to Bright ULXs"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T08:24:51.065202+00:00"}