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dc.contributor.authorPuerari, I.
dc.contributor.authorBlock, D.L.
dc.contributor.authorKnapen, J.
dc.contributor.authorElmegreen, B.
dc.contributor.authorButa, R.J.
dc.contributor.authorStedman, S.
dc.contributor.authorElmegreen, D.M.
dc.date.accessioned2008-01-30T10:38:13Z
dc.date.available2008-01-30T10:38:13Z
dc.date.issued2002
dc.identifier.citationPuerari , I , Block , D L , Knapen , J , Elmegreen , B , Buta , R J , Stedman , S & Elmegreen , D M 2002 , The Gravitational Torque of Bars . in In: Procs of Disks of Galaxies: Kinematics, Dynamics and Peturbations - ASP Conference Series 275 . Astronomical Society of the Pacific , pp. 193-196 .
dc.identifier.isbn1-58381-117-6
dc.identifier.otherPURE: 144992
dc.identifier.otherPURE UUID: 57f3663a-d47f-49af-bc52-aff083b631aa
dc.identifier.otherdspace: 2299/1457
dc.identifier.urihttp://hdl.handle.net/2299/1457
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/253.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe have determined the gravitational torque of a sample of 45 galaxies observed at K band with the 4.2m William Herschel Telescope. The results of this sample, combined with those for a sample of 30 galaxies previously analysed (Buta & Block 2001), show that the gravitational bar torque correlates only weakly with the optical bar type listed in the Revised Shapley-Ames and de Vaucouleurs systems. In fact, Some classically unbarred galaxies have larger bar torques than classically barred galaxies. The Hubble classification scheme poorly recognizes the gravitational influences of the bar perturbation in the force field.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of Disks of Galaxies: Kinematics, Dynamics and Peturbations - ASP Conference Series 275
dc.titleThe Gravitational Torque of Barsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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