{"@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/1360004239676657664.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/1538-4357/aaf9a9"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/871/i=2/a=257/pdf"}},{"identifier":{"@type":"URI","@value":"http://stacks.iop.org/0004-637X/871/i=2/a=257?key=crossref.b4ac18a25ad26c417c33e78810e49376"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/aaf9a9"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4357/aaf9a9/pdf"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Faraday Rotation in the Jet of M87 inside the Bondi Radius: Indication of Winds from Hot Accretion Flows Confining the Relativistic Jet"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>We study Faraday rotation in the jet of M87 inside the Bondi radius using eight Very Long Baseline Array data sets, one at 8 GHz, four at 5 GHz, and three at 2 GHz. We obtain Faraday rotation measures (RMs) measured across the bandwidth of each data set. We find that the magnitude of RM systematically decreases with increasing distance from 5000 to 200,000 Schwarzschild radii. The data, showing predominantly negative RM signs without significant difference of the RMs on the northern and southern jet edges, suggest that the spatial extent of the Faraday screen is much larger than the jet. We apply models of hot accretion flows, thought to be prevalent in active galactic nuclei with a relatively low luminosity such as M87, and find that the decrease of RM is described well by a gas density profile <jats:inline-formula>\n                     <jats:tex-math>\n\n</jats:tex-math>\n                     <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" xlink:href=\"apjaaf9a9ieqn1.gif\" xlink:type=\"simple\"/>\n                  </jats:inline-formula>. This behavior matches the theoretically expected signature of substantial winds, nonrelativistic un-collimated gas outflows from hot accretion flows, which is consistent with the results of various numerical simulations. The pressure profile inferred from the density profile is flat enough to collimate the jet, which can result in gradual acceleration of the jet in a magneto-hydrodynamical process. This picture is in good agreement with the observed gradual collimation and acceleration of the M87 jet inside the Bondi radius. The dominance of negative RMs suggests that the jet and wind axis are misaligned such that the jet emission exposes only one side of the toroidal magnetic fields permeating the winds.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380004239676658181","@type":"Researcher","foaf:name":[{"@value":"Jongho Park"}]},{"@id":"https://cir.nii.ac.jp/crid/1420282801210953472","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"60724458"},{"@type":"NRID","@value":"1000060724458"},{"@type":"NRID","@value":"9000370741055"},{"@type":"NRID","@value":"9000005445422"}],"foaf:name":[{"@value":"Kazuhiro Hada"}]},{"@id":"https://cir.nii.ac.jp/crid/1420001326224080256","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"70531234"},{"@type":"NRID","@value":"1000070531234"},{"@type":"NRID","@value":"9000364772813"},{"@type":"NRID","@value":"9000244901956"},{"@type":"NRID","@value":"9000351491237"},{"@type":"NRID","@value":"9000014651576"},{"@type":"NRID","@value":"9000244901853"},{"@type":"NRID","@value":"9000006551300"},{"@type":"NRID","@value":"9000279645151"}],"foaf:name":[{"@value":"Motoki Kino"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676657794","@type":"Researcher","foaf:name":[{"@value":"Masanori Nakamura"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676658061","@type":"Researcher","foaf:name":[{"@value":"Hyunwook Ro"}]},{"@id":"https://cir.nii.ac.jp/crid/1380004239676657675","@type":"Researcher","foaf:name":[{"@value":"Sascha Trippe"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"0004637X"},{"@type":"EISSN","@value":"15384357"}],"prism:publicationName":[{"@value":"The Astrophysical Journal"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2019-02-01","prism:volume":"871","prism:number":"2","prism:startingPage":"257"},"reviewed":"false","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"http://stacks.iop.org/0004-637X/871/i=2/a=257/pdf"},{"@id":"http://stacks.iop.org/0004-637X/871/i=2/a=257?key=crossref.b4ac18a25ad26c417c33e78810e49376"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/aaf9a9"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4357/aaf9a9/pdf"}],"createdAt":"2019-02-05","modifiedAt":"2024-01-12","project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781994065024","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18H03721"},{"@type":"JGN","@value":"JP18H03721"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18H03721/"}],"notation":[{"@language":"ja","@value":"直接撮像で探る巨大ブラックホール最近傍におけるガス噴出機構"},{"@language":"en","@value":"Study of launching mechanism of cosmic jet in the vicinity of super massive black-hole by direct imaging"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781998274560","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18K03656"},{"@type":"JGN","@value":"JP18K03656"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18K03656/"}],"notation":[{"@language":"ja","@value":"一般相対論的輻射輸送計算と電波VLBI観測で探るブラックホールジェットの駆動機構"},{"@language":"en","@value":"Study of driving mechanism of black hole jets by general relativistic radiative transfer and VLBI observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782006509568","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18KK0090"},{"@type":"JGN","@value":"JP18KK0090"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18KK0090/"}],"notation":[{"@language":"ja","@value":"地球規模電波望遠鏡ネットワークで挑む巨大ブラックホールジェット生成機構"},{"@language":"en","@value":"Revealing the formation of relativistic jets in supermassive black holes using global VLBI networks"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360002217424872320","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE INNERMOST COLLIMATION STRUCTURE OF THE M87 JET DOWN TO ∼10 SCHWARZSCHILD RADII"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217425689600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"230 GHz VLBI OBSERVATIONS OF M87: EVENT‐HORIZON‐SCALE STRUCTURE DURING AN ENHANCED VERY‐HIGH‐ENERGY $\\gamma $‐RAY STATE IN 2012"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217472320512","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DISCOVERY OF SUB- TO SUPERLUMINAL MOTIONS IN THE M87 JET: AN IMPLICATION OF ACCELERATION FROM SUB-RELATIVISTIC TO RELATIVISTIC 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