{"created":"2023-06-20T13:22:37.935911+00:00","id":3292,"links":{},"metadata":{"_buckets":{"deposit":"6893be5b-1a40-4f84-9c4e-20f02829be98"},"_deposit":{"created_by":21,"id":"3292","owners":[21],"pid":{"revision_id":0,"type":"depid","value":"3292"},"status":"published"},"_oai":{"id":"oai:ir.soken.ac.jp:00003292","sets":["1:274"]},"author_link":["734","736","737","735","738","739"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2000-06","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1","bibliographicPageEnd":"L7","bibliographicPageStart":"L1","bibliographicVolumeNumber":"315","bibliographic_titles":[{"bibliographic_title":"Monthly Notices of the Royal Astronomical Society"},{"bibliographic_title":"Monthly Notices of the Royal Astronomical Society","bibliographic_titleLang":"en"}]}]},"item_10001_creator_3":{"attribute_name":"著者別名","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"池内, 了"}],"nameIdentifiers":[{},{},{}]}]},"item_10001_description_19":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_10001_description_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"To explain the effects of the ultraviolet (UV) background radiation on the collapse of pre-galactic clouds, we implement a radiation–hydrodynamical calculation, combining one-dimensional spherical hydrodynamics with an accurate treatment of the radiative transfer of ionizing photons. Both absorption and scattering of UV photons are explicitly taken into account. It turns out that a gas cloud contracting within the dark matter potential does not settle into hydrostatic equilibrium, but undergoes run-away collapse even under the presence of the external UV field. The cloud centre is shown to become self-shielded against ionizing photons by radiative transfer effects before shrinking to the rotation barrier. Based on our simulation results, we further discuss the possibility of H2 cooling and subsequent star formation in a run-away collapsing core. The present results are closely relevant to the survival of subgalactic Population III objects as well as to metal injection into intergalactic space.","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Wiley"}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1046/j.1365-8711.2000.03589.x"}],"subitem_relation_type":"isIdenticalTo","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.1046/j.1365-8711.2000.03589.x","subitem_relation_type_select":"DOI"}}]},"item_10001_relation_17":{"attribute_name":"関連サイト","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"Copyright"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://www.blackwellpublishing.com/pdf/mnr_caf.pdf","subitem_relation_type_select":"URI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"©2000 The Royal Astronomical Society"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"00358711 ","subitem_source_identifier_type":"ISSN"}]},"item_10001_version_type_20":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_970fb48d4fbd8a85","subitem_version_type":"VoR"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"KITAYAMA, Tetsu"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"TAJIRI, Yukiko"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"UMEMURA, Masayuki"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"SUSA, Hajime"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"IKEUCHI, Satoru"}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2014-03-10"}],"displaytype":"simple","filename":"j.1365-8711.2000.03589.x.pdf","filesize":[{"value":"446.2 kB"}],"format":"application/pdf","licensetype":"license_11","mimetype":"application/pdf","url":{"label":"j.1365-8711.2000.03589.x","url":"https://ir.soken.ac.jp/record/3292/files/j.1365-8711.2000.03589.x.pdf"},"version_id":"f0f9a5e5-cc00-47df-b37f-2fdf268f2f73"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"radiative transfer,galaxies,formation,cosmology,theory,diffuse radiation","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":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"Radiation-hydrodynamical collapse of pre-galactic clouds in the ultraviolet background","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Radiation-hydrodynamical collapse of pre-galactic clouds in the ultraviolet background"},{"subitem_title":"Radiation-hydrodynamical collapse of pre-galactic clouds in the ultraviolet background","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"21","path":["95","274"],"pubdate":{"attribute_name":"公開日","attribute_value":"2012-12-13"},"publish_date":"2012-12-13","publish_status":"0","recid":"3292","relation_version_is_last":true,"title":["Radiation-hydrodynamical collapse of pre-galactic clouds in the ultraviolet background"],"weko_creator_id":"21","weko_shared_id":21},"updated":"2023-06-20T14:12:03.208462+00:00"}