An 8.4-GHz long baseline array observation of the unusual Seyfert galaxy NGC 7213

Blank, D; Harnett, JI; Jones, P

An 8.4-GHz long baseline array observation of the unusual Seyfert galaxy NGC 7213

Blank, D Harnett, JI Jones, P

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Publisher:: Blackwell Publishing Ltd
Publication Type:: Journal Article
Citation:: Monthly Notices Of The Royal Astronomical Society, 2005, 356 (2), pp. 734 - 736
Issue Date:: 2005-01

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Field	Value	Language
dc.contributor.author	Blank, D	en_US
dc.contributor.author	Harnett, JI	en_US
dc.contributor.author	Jones, P	en_US
dc.date.issued	2005-01	en_US
dc.identifier.citation	Monthly Notices Of The Royal Astronomical Society, 2005, 356 (2), pp. 734 - 736	en_US
dc.identifier.issn	0035-8711	en_US
dc.identifier.uri	http://hdl.handle.net/10453/357
dc.description.abstract	We have observed the type 1.5 Seyfert galaxy NGC 7213 with the Australian Long Baseline Array (LBA) at 8.4 GHz to discover whether this object has the high brightness temperature compact core suggested by low-frequency variability. Confirmation would sup	en_US
dc.publisher	Blackwell Publishing Ltd	en_US
dc.relation.ispartof	Monthly Notices Of The Royal Astronomical Society	en_US
dc.relation.isbasedon	10.1111/j.1365-2966.2004.08506.x	en_US
dc.subject.classification	Astronomy & Astrophysics	en_US
dc.title	An 8.4-GHz long baseline array observation of the unusual Seyfert galaxy NGC 7213	en_US
dc.type	Journal Article
utslib.citation.volume	2	en_US
utslib.citation.volume	356	en_US
utslib.for	0201 Astronomical and Space Sciences	en_US
pubs.embargo.period	Not known	en_US
pubs.organisational-group	/University of Technology Sydney
pubs.organisational-group	/University of Technology Sydney/Faculty of Engineering and Information Technology
pubs.organisational-group	/University of Technology Sydney/Faculty of Engineering and Information Technology/School of Electrical and Data Engineering
utslib.copyright.status	open_access
pubs.consider-herdc	true	en_US
pubs.issue	2	en_US
pubs.volume	356	en_US

Abstract:

We have observed the type 1.5 Seyfert galaxy NGC 7213 with the Australian Long Baseline Array (LBA) at 8.4 GHz to discover whether this object has the high brightness temperature compact core suggested by low-frequency variability. Confirmation would sup

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http://hdl.handle.net/10453/357