{"created":"2021-03-01T07:16:33.992972+00:00","id":37452,"links":{},"metadata":{"_buckets":{"deposit":"5cc28d14-ef77-496b-ab1e-eddc81c35d73"},"_deposit":{"id":"37452","owners":[],"pid":{"revision_id":0,"type":"depid","value":"37452"},"status":"published"},"_oai":{"id":"oai:tsukuba.repo.nii.ac.jp:00037452","sets":["3048:1203","3:62:5296:4998"]},"item_5_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2016-02","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"1-2","bibliographicPageEnd":"174","bibliographicPageStart":"167","bibliographicVolumeNumber":"337","bibliographic_titles":[{"bibliographic_title":"Astronomische nachrichten"}]}]},"item_5_creator_3":{"attribute_name":"著者別名","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Wagner, Alexander"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"梅村, 雅之"}],"nameIdentifiers":[{},{},{}]}]},"item_5_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"Powerful relativistic jets in radio galaxies are capable of driving strong outflows but also inducing star-formation by pressure-triggering collapse of dense clouds. We review theoretical work on negative and positive active galactic nuclei feedback, discussing insights gained from recent hydrodynamical simulations of jet-driven feedback on galaxy scales that are applicable to compact radio sources. The simulations show that the efficiency of feedback and the relative importance of negative and positive feedback depend strongly on interstellar medium properties, especially the column depth and spatial distribution of clouds. Negative feedback is most effective if clouds are distributed spherically and individual clouds have small column depths, while positive feedback is most effective if clouds are predominantly in a disc-like configuration.","subitem_description_type":"Abstract"}]},"item_5_publisher_27":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"Wiley"}]},"item_5_relation_11":{"attribute_name":"DOI","attribute_value_mlt":[{"subitem_relation_type_id":{"subitem_relation_type_id_text":"10.1002/asna.201512287","subitem_relation_type_select":"DOI"}}]},"item_5_rights_12":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"© 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim "},{"subitem_rights":"This is the peer reviewed version of the following article: Astronomische Nachrichten Volume 337, Issue 1-2, pages 167–174, February 2016, which has been published in final form at http://onlinelibrary.wiley.com/doi/10.1002/asna.201512287. This article may be used for non-commercial purposes in accordance with Wiley Terms and Conditions for Self-Archiving."}]},"item_5_select_15":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_select_item":"author"}]},"item_5_source_id_7":{"attribute_name":"ISSN","attribute_value_mlt":[{"subitem_source_identifier":"0004-6337","subitem_source_identifier_type":"ISSN"}]},"item_5_source_id_9":{"attribute_name":"書誌レコードID","attribute_value_mlt":[{"subitem_source_identifier":"AA00553129","subitem_source_identifier_type":"NCID"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"Wagner, A. Y."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Bicknell, G. V."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Umemura, M."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Sutherland, R. S."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Silk, J."}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2017-03-01"}],"displaytype":"detail","filename":"AN_337-1-2.pdf","filesize":[{"value":"5.8 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"AN_337-1-2","url":"https://tsukuba.repo.nii.ac.jp/record/37452/files/AN_337-1-2.pdf"},"version_id":"0710a076-211d-49bc-9e83-54cc9d8e5ab3"}]},"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":"Galaxy-scale AGN feedback – theory","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Galaxy-scale AGN feedback – theory"}]},"item_type_id":"5","owner":"1","path":["1203","4998"],"pubdate":{"attribute_name":"公開日","attribute_value":"2016-03-22"},"publish_date":"2016-03-22","publish_status":"0","recid":"37452","relation_version_is_last":true,"title":["Galaxy-scale AGN feedback – theory"],"weko_creator_id":"1","weko_shared_id":5},"updated":"2022-04-27T09:07:04.654773+00:00"}