{"created":"2023-07-27T04:39:33.905110+00:00","id":12245,"links":{},"metadata":{"_buckets":{"deposit":"d2639536-9162-45dc-8b43-135ddc26fa51"},"_deposit":{"created_by":3,"id":"12245","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"12245"},"status":"published"},"_oai":{"id":"oai:tohoku.repo.nii.ac.jp:00012245","sets":["91:156"]},"author_link":["26790","26791"],"item_4_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1987-03-20","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"3","bibliographicPageEnd":"231","bibliographicPageStart":"217","bibliographicVolumeNumber":"7","bibliographic_titles":[{"bibliographic_title":"The science reports of the Tohoku University. Ser. 8, Physics and astronomy"}]}]},"item_4_date_62":{"attribute_name":"登録日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-05-02","subitem_date_issued_type":"Created"}]},"item_4_date_63":{"attribute_name":"公開日（投稿完了日）","attribute_value_mlt":[{"subitem_date_issued_datetime":"2008-05-02","subitem_date_issued_type":"Created"}]},"item_4_date_65":{"attribute_name":"発行日","attribute_value_mlt":[{"subitem_date_issued_datetime":"1987-03-20","subitem_date_issued_type":"Created"}]},"item_4_date_80":{"attribute_name":"更新日","attribute_value_mlt":[{"subitem_date_issued_datetime":"2010-01-27","subitem_date_issued_type":"Created"}]},"item_4_description_15":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"application/pdf","subitem_description_type":"Other"}]},"item_4_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"The interstellar medium is observed to be fragmented at all scales ranging from that of the supercloud complexes to that of the protostellar cores, forming a hierarchy which is not self-similar. In the solar neighbourhood, the self-similarity breaks down at a salient scale which we call that of 'clouds': their mass is several 100M_<&odot;>, their size a few parsecs. The clouds, building blocks of the hierarchy, are supported against gravity by supersonic but subalfvenic turbulence. We show that this turbulence can be fed, via magnetohydrodynamic waves, over several 10^7 years, by a pumping of the orbital kinetic energy of the other clouds within the same complex. We also show that local gravitational instabilities may develop within the gravitationally stable clouds and eventually form dense protostellar cores.","subitem_description_type":"Abstract"}]},"item_4_description_41":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"subitem_description":"紀要類(bulletin)","subitem_description_type":"Other"}]},"item_4_description_66":{"attribute_name":"フォーマット","attribute_value_mlt":[{"subitem_description":"958936 bytes","subitem_description_type":"Other"}]},"item_4_publisher_34":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Faculty of Science, Tohoku University"}]},"item_4_radio_69":{"attribute_name":"公開範囲","attribute_value_mlt":[{"subitem_radio_item":"学外"}]},"item_4_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"03885607","subitem_source_identifier_type":"ISSN"}]},"item_4_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00441828","subitem_source_identifier_type":"NCID"}]},"item_4_version_type_16":{"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":"Falgarone, E."}],"nameIdentifiers":[{"nameIdentifier":"26790","nameIdentifierScheme":"WEKO"}]},{"creatorNames":[{"creatorName":"Perault, M."}],"nameIdentifiers":[{"nameIdentifier":"26791","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":"2017-02-03"}],"displaytype":"detail","filename":"KJ00004430027.pdf","filesize":[{"value":"958.9 kB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"KJ00004430027.pdf","url":"https://tohoku.repo.nii.ac.jp/record/12245/files/KJ00004430027.pdf"},"version_id":"d6439756-9b36-42b0-83ca-bf80d117bc48"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Radioastronomie millimetrique","subitem_subject_scheme":"Other"},{"subitem_subject":"Ecole Normals Superieure","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":"departmental bulletin paper","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"STRUCTURE AND PHYSICS OF COOL GIANT MOLECULAR COMPLEXES(Proceedings of Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation)","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"STRUCTURE AND PHYSICS OF COOL GIANT MOLECULAR COMPLEXES(Proceedings of Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation)"}]},"item_type_id":"4","owner":"3","path":["156"],"pubdate":{"attribute_name":"公開日","attribute_value":"2008-05-02"},"publish_date":"2008-05-02","publish_status":"0","recid":"12245","relation_version_is_last":true,"title":["STRUCTURE AND PHYSICS OF COOL GIANT MOLECULAR COMPLEXES(Proceedings of Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation)"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2023-07-27T12:33:31.251623+00:00"}