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dc.contributor.authorAllard, E.L.
dc.contributor.authorPeletier, R.F.
dc.contributor.authorKnapen, J.
dc.identifier.citationAllard , E L , Peletier , R F & Knapen , J 2005 , Stellar and Gas Kinematics in the core and bar regions of M100 . in The Evolution of Star Bursts : the 331st Wilhelm & Else Heraeus Seminar . AIP Conf Procs , vol. 783 , American Institute of Physics , pp. 72-75 .
dc.identifier.otherPURE: 463104
dc.identifier.otherPURE UUID: 631892eb-3f7a-40c6-b77e-bc200477c1eb
dc.identifier.otherdspace: 2299/3696
dc.identifier.otherScopus: 33749554182
dc.descriptionOriginal paper can be found at Copyright American Institute of Physics. DOI: 10.1063/1.2034969 [Full text of this article is not available in the UHRA]
dc.description.abstractTwo-dimensional maps of the stellar and gas kinematics of the bar and starbursting circumnuclear region in the barred spiral galaxy M100 are presented. In this progress report, we present maps of the total intensity, mean velocity and velocity dispersion for the stars and the gas. The gas velocity field shows significant kinematic signatures of gas streaming along the inner part of the bar, and across the miniature spiral arms in the nuclear pseudo-ring. The stellar velocity field, presented here for the first time, also shows non-circular motions. The gas velocity dispersion is notably smaller where the star formation occurs in the nuclear zone and HII regions. We outline our further plans with the data set.en
dc.publisherAmerican Institute of Physics
dc.relation.ispartofThe Evolution of Star Bursts
dc.relation.ispartofseriesAIP Conf Procs
dc.titleStellar and Gas Kinematics in the core and bar regions of M100en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics

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