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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2399

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DC Field	Value	Language
dc.contributor.author	Tateyama, Claudio E.	-
dc.contributor.author	Dhawan, V.	-
dc.contributor.author	et al.	-
dc.date.accessioned	2007-05-25T08:02:02Z	-
dc.date.available	2007-05-25T08:02:02Z	-
dc.date.issued	1996-02	-
dc.identifier.citation	Publications of the Astronomical Society of Japan, 1996, Vol.48, p37-44	en
dc.identifier.issn	0004-6264	-
dc.identifier.uri	http://hdl.handle.net/2289/2399	-
dc.description	Restricted Access.	en
dc.description.abstract	We 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.extent	967430 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of Japan	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?1996PASJ...48...37T	en
dc.rights	1996 Astronomical Society of Japan	en
dc.subject	BL LACERTAE OBJECTS	en
dc.subject	GALAXIES: ACTIVE	en
dc.subject	GALAXIES: INDIVIDUAL (OJ 287)	en
dc.subject	RADIO SOURCES: VARIABLE	en
dc.title	Global 3- and 7-mm VLBI observations of OJ 287	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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