{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1363670320843644544.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1126/science.1240436"}},{"identifier":{"@type":"URI","@value":"https://www.science.org/doi/pdf/10.1126/science.1240436"}}],"dc:title":[{"@value":"Radio Jets Clearing the Way Through a Galaxy: Watching Feedback in Action"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Pushy Black Hole</jats:title>\n          <jats:p>\n            The giant black holes that sit at the centers of most galaxies influence the way galaxies evolve in poorly understood ways.\n            <jats:bold>\n              Morganti\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" issue=\"6150\" page=\"1082\" related-article-type=\"in-this-issue\" vol=\"341\" xlink:href=\"10.1126/science.1240436\">1082</jats:related-article>\n            ; see the Perspective by\n            <jats:bold>\n              <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" issue=\"6150\" page=\"1073\" related-article-type=\"in-this-issue\" vol=\"341\" xlink:href=\"10.1126/science.1243114\">McNamara</jats:related-article>\n            </jats:bold>\n            ) have acquired high-resolution radio images of a galaxy with an actively accreting black hole from which a jet of relativistic particles emanates. The observations show that a cloud of neutral hydrogen gas is being driven outward, possibly limiting star formation and galaxy growth.\n          </jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1383670320843644545","@type":"Researcher","foaf:name":[{"@value":"Raffaella Morganti"}],"jpcoar:affiliationName":[{"@value":"ASTRON, Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands."},{"@value":"Kapteyn Astronomical Institute, University of Groningen, Post Office Box 800, 9700 AV Groningen, Netherlands."}]},{"@id":"https://cir.nii.ac.jp/crid/1383670320843644546","@type":"Researcher","foaf:name":[{"@value":"Judit Fogasy"}],"jpcoar:affiliationName":[{"@value":"Eötvös Loránd University, Egyetem tér 1-3, 1053 Budapest, Hungary."}]},{"@id":"https://cir.nii.ac.jp/crid/1383670320843644544","@type":"Researcher","foaf:name":[{"@value":"Zsolt Paragi"}],"jpcoar:affiliationName":[{"@value":"Joint Institute for Very Long Baseline Interferometry (VLBI) in Europe, Postbus 2, 7990 AA Dwingeloo, Netherlands."}]},{"@id":"https://cir.nii.ac.jp/crid/1383670320843644547","@type":"Researcher","foaf:name":[{"@value":"Tom Oosterloo"}],"jpcoar:affiliationName":[{"@value":"ASTRON, Netherlands Institute for Radio Astronomy, Postbus 2, 7990 AA, Dwingeloo, Netherlands."},{"@value":"Kapteyn Astronomical Institute, University of Groningen, Post Office Box 800, 9700 AV Groningen, Netherlands."}]},{"@id":"https://cir.nii.ac.jp/crid/1383670320843644548","@type":"Researcher","foaf:name":[{"@value":"Monica Orienti"}],"jpcoar:affiliationName":[{"@value":"Istituto Nazionale di Astrofisica (INAF)–Istituto di Radioastronomia, via Gobetti 101, I-40129, Bologna, Italy."}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00368075"},{"@type":"EISSN","@value":"10959203"}],"prism:publicationName":[{"@value":"Science"}],"dc:publisher":[{"@value":"American Association for the Advancement of Science (AAAS)"}],"prism:publicationDate":"2013-09-06","prism:volume":"341","prism:number":"6150","prism:startingPage":"1082","prism:endingPage":"1085"},"reviewed":"false","url":[{"@id":"https://www.science.org/doi/pdf/10.1126/science.1240436"}],"createdAt":"2013-09-05","modifiedAt":"2024-01-10","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050005987800500096","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). 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The Optical Counterparts of FIRST Radio Sources"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643732236928","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Morphological Transition of the Compact Radio Lobe in 3C 84 via the Strong Jet–Cloud Collision"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568469552268672","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Searching for signs of jet-driven negative feedback in the nearby radio galaxy UGC 05771"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118750904960","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Impact of relativistic jets on the star formation rate: a turbulence-regulated framework"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846645714753536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Feeding and Feedback in the Powerful Radio Galaxy 3C 120"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865818707345920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"<i>RadioAstron</i>discovery of a mini-cocoon around the restarted parsec-scale jet in 3C 84"}]},{"@id":"https://cir.nii.ac.jp/crid/1361131419505658496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Jets blowing bubbles in the young radio galaxy 4C 31.04"}]},{"@id":"https://cir.nii.ac.jp/crid/1363383444217639424","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The ALMA Discovery of the Rotating Disk and Fast Outflow of Cold Molecular Gas in NGC 1275"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1126/science.1240436"},{"@type":"CROSSREF","@value":"10.1017/s174392131500201x_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aae1ac_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/ac24fa_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.1093/mnras/stz2459_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ab238d_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.3847/1538-3881/ab98fe_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.1093/mnras/stab2822_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/aa6342_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202142594_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.1093/mnras/stz233_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ab3e6e_references_DOI_C3uxorSN3iAONnQwBIUh4Eu5ZDP"}]}