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dc.contributor.authorKnapen, J.
dc.date.accessioned2009-07-21T13:22:31Z
dc.date.available2009-07-21T13:22:31Z
dc.date.issued2005
dc.identifier.citationKnapen , J 2005 , ' Barred galaxies : Stars and Bars ' , Astronomy and Geophysics , vol. 46 , no. 6 , pp. 28-33 . https://doi.org/10.1111/j.1468-4004.2005.46628.x
dc.identifier.issn1366-8781
dc.identifier.otherPURE: 161424
dc.identifier.otherPURE UUID: c2880d36-f5cc-41eb-83b4-005eface7f14
dc.identifier.otherdspace: 2299/3691
dc.identifier.otherScopus: 28744440455
dc.identifier.urihttp://hdl.handle.net/2299/3691
dc.description‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1468-4004.2005.46628.x [Full text of this article is not available in the UHRA]
dc.description.abstractBars are prominent features that occur in most disc galaxies and have important dynamical effects on their hosts. This paper describes some of the known properties of bars, illustrating the discussion with images that show the beauty of the galaxies under consideration. The focus of this article is on the evolution of bars and on their influence on the redistribution of matter within galaxies. In this way, bars drive the internal, or secular, evolution of galaxies.en
dc.language.isoeng
dc.relation.ispartofAstronomy and Geophysics
dc.titleBarred galaxies : Stars and Barsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted2005
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1468-4004.2005.46628.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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