Kinematics of the Circumnuclear Region of M 100

dc.contributor.author	Knapen, J.
dc.contributor.editor	Combes, F.
dc.contributor.editor	Mamon, G.A.
dc.contributor.editor	Charmandaris, V.
dc.date.accessioned	2011-11-15T17:01:05Z
dc.date.available	2011-11-15T17:01:05Z
dc.date.issued	2000
dc.identifier.citation	Knapen , 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.other	dspace: 2299/434
dc.identifier.uri	http://hdl.handle.net/2299/7019
dc.description.abstract	Circumnuclear 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.format.extent	447993
dc.language.iso	eng
dc.publisher	Astronomical Society of the Pacific
dc.relation.ispartof	Dynamics of Galaxies
dc.relation.ispartofseries	ASP Conf Series
dc.title	Kinematics of the Circumnuclear Region of M 100	en
dc.contributor.institution	School of Physics, Astronomy and Mathematics
rioxxterms.type	Other
herts.preservation.rarelyaccessed	true