{"created":"2023-06-19T09:12:41.217733+00:00","id":24553,"links":{},"metadata":{"_buckets":{"deposit":"8667a176-87b1-4b83-a763-2bfdd2829d61"},"_deposit":{"created_by":12,"id":"24553","owners":[12],"pid":{"revision_id":0,"type":"depid","value":"24553"},"status":"published"},"_oai":{"id":"oai:kumadai.repo.nii.ac.jp:00024553","sets":["448:538","585:614:1055"]},"author_link":["155854","155859","155811"],"item_15_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2010","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"182","bibliographicPageStart":"171","bibliographicVolumeNumber":"13","bibliographic_titles":[{"bibliographic_title":"Physics Reports of Kumamoto University","bibliographic_titleLang":"en"}]}]},"item_15_description_5":{"attribute_name":"内容記述","attribute_value_mlt":[{"subitem_description":"We investigate the two-temperature model of the Advection Dominated Accretion Flow (ADAF) around a supermassive black hole. Electron temperature is determined from the local balance between energy transfer from ions through Coulomb collisions and radiative cooling via bremsstrahlung, synchrotron radiation and inverse Compton scattering. Appling our model to Sgr A*, we evaluate the corresponding spectrum emitted from the whole disk. It is found that the resulting spectrum is well fitted to the observed one when the mass accretion rate is in the range (3.6-7.2) x10^-8 M_sun yr^-1, which is in agreement with the value derived from polarized emission at radio wavelength.","subitem_description_language":"en","subitem_description_type":"Other"}]},"item_15_publisher_36":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"熊本大学","subitem_publisher_language":"ja"}]},"item_15_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0303-4070","subitem_source_identifier_type":"PISSN"}]},"item_15_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00774081","subitem_source_identifier_type":"NCID"}]},"item_15_subject_20":{"attribute_name":"日本十進分類法","attribute_value_mlt":[{"subitem_subject":"443.5","subitem_subject_scheme":"NDC"}]},"item_15_version_type_19":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Baba, Tamon","creatorNameLang":"en"},{"creatorName":"馬場, 多聞","creatorNameLang":"ja"},{"creatorName":"ババ, タモン","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"155854","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Kai, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{"nameIdentifier":"155859","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Arai, Kenzo","creatorNameLang":"en"},{"creatorName":"荒井, 賢三","creatorNameLang":"ja"},{"creatorName":"アライ, ケンゾウ","creatorNameLang":"ja-Kana"}],"nameIdentifiers":[{"nameIdentifier":"155811","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":"2020-03-02"}],"displaytype":"detail","filename":"PR0013_171-182.pdf","filesize":[{"value":"2.2 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"PR0013_171-182.pdf","url":"https://kumadai.repo.nii.ac.jp/record/24553/files/PR0013_171-182.pdf"},"version_id":"6a2ffed4-f459-4d41-9b42-c1977ca7707a"}]},"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":"Two-Temperature Model of Advection Dominated Accretion Flow","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Two-Temperature Model of Advection Dominated Accretion Flow","subitem_title_language":"en"}]},"item_type_id":"15","owner":"12","path":["538","1055"],"pubdate":{"attribute_name":"PubDate","attribute_value":"2011-02-23"},"publish_date":"2011-02-23","publish_status":"0","recid":"24553","relation_version_is_last":true,"title":["Two-Temperature Model of Advection Dominated Accretion Flow"],"weko_creator_id":"12","weko_shared_id":-1},"updated":"2023-10-17T06:40:17.393709+00:00"}