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Global 3- and 7-mm VLBI observations of OJ 287

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dc.contributor.authorTateyama, Claudio E.
dc.contributor.authorDhawan, V.
dc.contributor.authoret al.
dc.date.accessioned2007-05-25T08:02:02Z
dc.date.available2007-05-25T08:02:02Z
dc.date.issued1996-02
dc.descriptionRestricted Access.en
dc.description.abstractWe present new results from global VLBI observations of the highly active blazar OJ 287 at 7 and 3 mm wavelengths. We show the first map of the mas to sub-mas structure of OJ 287 at 43 GHz and discuss this image in the context with models of the source structure seen at 100 GHz.en
dc.format.extent967430 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationPublications of the Astronomical Society of Japan, 1996, Vol.48, p37-44en
dc.identifier.issn0004-6264
dc.identifier.urihttp://hdl.handle.net/2289/2399
dc.language.isoenen
dc.publisherAstronomical Society of Japanen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1996PASJ...48...37Ten
dc.rights1996 Astronomical Society of Japanen
dc.subjectBL LACERTAE OBJECTSen
dc.subjectGALAXIES: ACTIVEen
dc.subjectGALAXIES: INDIVIDUAL (OJ 287)en
dc.subjectRADIO SOURCES: VARIABLEen
dc.titleGlobal 3- and 7-mm VLBI observations of OJ 287en
dc.typeArticleen

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