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dc.contributor.authorKnapen, J.
dc.contributor.editorCombes, F.
dc.contributor.editorMamon, G.A.
dc.contributor.editorCharmandaris, V.
dc.date.accessioned2011-11-15T17:01:05Z
dc.date.available2011-11-15T17:01:05Z
dc.date.issued2000
dc.identifier.citationKnapen , J 2000 , Kinematics of the Circumnuclear Region of M 100 . in F Combes , G A Mamon & V Charmandaris (eds) , Dynamics of Galaxies : from the Early Universe to the Present . vol. 197 , ASP Conf Series , vol. 197 , Astronomical Society of the Pacific , pp. 35-38 .
dc.identifier.otherPURE: 452564
dc.identifier.otherPURE UUID: 06cb499d-4202-4209-a5b0-5ea1bdc3679c
dc.identifier.otherdspace: 2299/434
dc.identifier.urihttp://hdl.handle.net/2299/7019
dc.description.abstractCircumnuclear regions of barred galaxies can host ring-like regions of enhanced star formation, thought to be related to the position of one or more Inner Lindblad resonance(s). Here we present kinematic observations and modelling of one such region, namely in the barred galaxy M100. The observations and modelling agree qualitatively and quantitatively, and support the idea that the circumnuclear structure forms an integral part of the dynamical structure of this galaxy.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofDynamics of Galaxies
dc.relation.ispartofseriesASP Conf Series
dc.rightsOpen
dc.titleKinematics of the Circumnuclear Region of M 100en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dc.description.versiontypeFinal Published version
dcterms.dateAccepted2000
rioxxterms.versionVoR
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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