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dc.contributor.authorCostantin, L.
dc.contributor.authorCorsini, E.M.
dc.contributor.authorMendez Abreu, Jairo
dc.contributor.authorBontà, E.D.
dc.contributor.authorMorelli, L.
dc.contributor.authorPizzella, A.
dc.date.accessioned2015-02-02T16:01:06Z
dc.date.available2015-02-02T16:01:06Z
dc.date.issued2014-12-12
dc.identifier.citationCostantin , L , Corsini , E M , Mendez Abreu , J , Bontà , E D , Morelli , L & Pizzella , A 2014 , ' The intrinsic shape and dynamical structure of the bulges of lenticular galaxies ' , Journal of Physics: Conference Series , vol. 566 , no. 1 , 012009 . https://doi.org/10.1088/1742-6596/566/1/012009en
dc.identifier.issn1742-6588
dc.identifier.otherPURE: 163649801
dc.identifier.otherPURE UUID: ece35659-1787-4336-af5c-6192a8b4f86a
dc.identifier.otherScopus: 84920053907
dc.identifier.otherWOS: 000347870900009
dc.identifier.urihttp://hdl.handle.net/10023/6057
dc.descriptionThis work was supported by Padua University through grants 60A02-5052/11, 60A02-4807/12, 60A02-5857/13, and CPDA133894. J.M.A. acknowledges support from the European Research Council Starting Grant (SEDmorph; P.I. V. Wild). L.M. received financial support from Padua University grant CPS0204.en
dc.description.abstractSeveral scenarios have been proposed to account for the formation and evolution of galactic bulges and to explain the variety of their observed properties. Both the intrinsic shape and dynamical structure of bulges depend on the mechanisms and timescales of their formation. We are deriving the intrinsic axial ratios of the bulges of a sample of unbarred lenticular galaxies to look for a possible relationship with their known orbital structure. Preliminary results show that the orbits of stars of the triaxial bulge of NGC 4476 are more anisotropic than those in the axisymmetric bulge of NGC 4249 hinting at a different formation process.
dc.language.isoeng
dc.relation.ispartofJournal of Physics: Conference Seriesen
dc.rightsCopyright 2014, The Authors. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence (http://creativecommons.org/licenses/by/3.0). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.en
dc.subjectQC Physicsen
dc.subjectQB Astronomyen
dc.subject.lccQCen
dc.subject.lccQBen
dc.titleThe intrinsic shape and dynamical structure of the bulges of lenticular galaxiesen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/1742-6596/566/1/012009
dc.description.statusPeer revieweden


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