Structure of the inner jet of OJ287 from VLBA data at 15 GHz in super-resolution mode

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dc.contributor.authorTateyama C.E.
dc.date.accessioned2024-03-13T01:04:58Z
dc.date.available2024-03-13T01:04:58Z
dc.date.issued2013
dc.description.abstractIn this work we show the results obtained from the Very Long Baseline Array data at 15 GHz of OJ287 in super-resolution mode. The data showed a jet configuration in the form of a "fork" where superluminal components emerge via stationary components at the northwest and the southeast close to the core to form parallel trajectories along the southwest direction in the plane of sky. This agrees with a source structure of an extended, broad morphology of OJ287. © 2013. The American Astronomical Society. All rights reserved..
dc.description.issuenumber2
dc.description.volume205
dc.identifier.doi10.1088/0067-0049/205/2/15
dc.identifier.issn0067-0049
dc.identifier.urihttps://dspace.mackenzie.br/handle/10899/36633
dc.relation.ispartofAstrophysical Journal, Supplement Series
dc.rightsAcesso Restrito
dc.subject.otherlanguageBL Lacertae objects: individual (OJ287)
dc.subject.otherlanguagegalaxies: jets
dc.subject.otherlanguageradio continuum: galaxies
dc.subject.otherlanguagetechniques: interferometric
dc.titleStructure of the inner jet of OJ287 from VLBA data at 15 GHz in super-resolution mode
dc.typeArtigo
local.scopus.citations8
local.scopus.eid2-s2.0-84875956098
local.scopus.updated2024-05-01
local.scopus.urlhttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=84875956098&origin=inward
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