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dc.contributor.authorKnapen, J.
dc.contributor.authorShlosman, I.
dc.contributor.authorBeckman, J.E.
dc.contributor.authorHeller, C.H.
dc.contributor.authorPeletier, R.F.
dc.contributor.authorde Jong, R.S.
dc.contributor.authorNadeau, D.
dc.contributor.authorDoyon, R.
dc.date.accessioned2008-02-05T12:10:41Z
dc.date.available2008-02-05T12:10:41Z
dc.date.issued1996
dc.identifier.citationKnapen , J , Shlosman , I , Beckman , J E , Heller , C H , Peletier , R F , de Jong , R S , Nadeau , D & Doyon , R 1996 , M100 and NGC 6951: Morphological Clues to Central Dynamics . in In: Barred galaxies, ASP Conference Series 91 . Astronomical Society of the Pacific , pp. 416-9 .
dc.identifier.isbn1-886733-12-0
dc.identifier.otherdspace: 2299/1554
dc.identifier.urihttp://hdl.handle.net/2299/1554
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific
dc.description.abstractHigh-resolution optical and NIR observations are used to constrain a dynamical model of the circumnuclear star forming (SF) region in the barred galaxy M100 (NGC 4321). Small leading arms observed in our K-band image of the nuclear region have been reproduced in numerical modeling of M100, a galaxy with a double inner Lindblad resonance (ILR). We also present preliminary optical and NIR observations of NGC 6951: a barred galaxy with circumnuclear SF showing a distinctly different behavior to M100 at 2.2um.en
dc.format.extent392856
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Barred galaxies, ASP Conference Series 91
dc.titleM100 and NGC 6951: Morphological Clues to Central Dynamicsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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