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dc.contributor.authorKnapen, J.
dc.contributor.authorLaine, S.
dc.contributor.authorShlosman, I.
dc.contributor.authorPeletier, R.F.
dc.date.accessioned2008-01-30T10:38:11Z
dc.date.available2008-01-30T10:38:11Z
dc.date.issued2003
dc.identifier.citationKnapen , J , Laine , S , Shlosman , I & Peletier , R F 2003 , Bars and Seyferts . in In: Procs of Active Galactic Nuclei: from Central Engine to Host Galaxy - ASP Conf Series 290 . Astronomical Society of the Pacific , pp. 419-422 .
dc.identifier.isbn1-58381-135-4
dc.identifier.otherdspace: 2299/1454
dc.identifier.urihttp://hdl.handle.net/2299/1454
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/286.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe describe the results of two studies recently undertaken, aimed at quantifying the properties of single and nested stellar bars in well-matched samples of Seyfert and non-Seyfert galaxies. We find that Seyfert host galaxies are more often barred than non-Seyferts. Sub-kpc bars in nested systems are probably confined to within the inner Lindblad resonance(s), and have a different formation and evolution history from large-scale bars. we do not find a substantial prevalence of stellar sub-kpc bars in Seyferts.en
dc.format.extent402058
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Active Galactic Nuclei: from Central Engine to Host Galaxy - ASP Conf Series 290
dc.titleBars and Seyfertsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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