{"created":"2023-06-20T13:22:55.125472+00:00","id":3643,"links":{},"metadata":{"_buckets":{"deposit":"3610277d-38cd-4d78-b1f7-dddf862b4316"},"_deposit":{"created_by":21,"id":"3643","owners":[21],"pid":{"revision_id":0,"type":"depid","value":"3643"},"status":"published"},"_oai":{"id":"oai:ir.soken.ac.jp:00003643","sets":["1:274"]},"author_link":["734","738"],"item_10001_biblio_info_7":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1991","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"246","bibliographicPageStart":"245","bibliographicVolumeNumber":"11","bibliographic_titles":[{"bibliographic_title":"Advances in Space Research "},{"bibliographic_title":"Advances in Space Research ","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_5":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"It is proposed that the HI absorption systems in quasars such as the Lyman α forest, Lyman limit systems and damped Lyman α lines are unifiedly understood based upon the expanding clouds confined by the gravity of cold dark matter (CDM). The correlation between these absorption systems and galaxy formation is discussed from the viewpoint of CDM cosmogony.","subitem_description_type":"Abstract"}]},"item_10001_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Elsevier"}]},"item_10001_relation_14":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_name":[{"subitem_relation_name_text":"10.1016/0273-1177(91)90497-8"}],"subitem_relation_type_id":{"subitem_relation_type_id_text":"http://doi.org/10.1016/0273-1177(91)90497-8 ","subitem_relation_type_select":"DOI"}}]},"item_10001_rights_15":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 1991 Published by Elsevier Ltd"}]},"item_10001_source_id_9":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"02731177 ","subitem_source_identifier_type":"ISSN"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"IKEUCHI, Satoru"}],"nameIdentifiers":[{}]}]},"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":"The nature of HI absorption systems at large redshifts","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The nature of HI absorption systems at large redshifts"},{"subitem_title":"The nature of HI absorption systems at large redshifts","subitem_title_language":"en"}]},"item_type_id":"10001","owner":"21","path":["274"],"pubdate":{"attribute_name":"公開日","attribute_value":"2013-06-27"},"publish_date":"2013-06-27","publish_status":"0","recid":"3643","relation_version_is_last":true,"title":["The nature of HI absorption systems at large redshifts"],"weko_creator_id":"21","weko_shared_id":21},"updated":"2023-06-20T14:31:54.230806+00:00"}