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Conference Paper: Galactic kinematics from RAVE to Gaia-RVS Data

TitleGalactic kinematics from RAVE to Gaia-RVS Data
Authors
Veltz, LBienaymé, OSteinmetz, MZwitter, TWatson, FGBinney, JBland-Hawthorn, JCampbell, RFreeman, KCGibson, BGilmore, GGrebel, EKHelmi, AMunari, UNavarro, JFParker, QASeabroke, GSiebert, ASiviero, AWilliams, MWyse, RFGCombes, FSamadi, R
Editors
Editor(s):Charbonnel, C
Issue Date2008
Citation
SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Paris, France, 30 June - 4 July 2008, p. 47-47 How to Cite?
AbstractRAVE data has provided new results on Galactic kinematics like the kinematical decomposition of the Galactic disk. This decomposition permits to identify the different components of the disk and to characterize them in terms of scale height and scale length. With the data provided by Gaia and in particular the RVS, we will have a completly renewed view of the Galaxy. The precision of the RVS will permit to undertake a precise analysis of the kinematics of the Galactic disks. This knowledge will provide significant clues to constrain the scenarios of the Galactic disk formation.
Persistent Identifierhttp://hdl.handle.net/10722/211250

 

DC FieldValueLanguage
dc.contributor.authorVeltz, L-
dc.contributor.authorBienaymé, O-
dc.contributor.authorSteinmetz, M-
dc.contributor.authorZwitter, T-
dc.contributor.authorWatson, FG-
dc.contributor.authorBinney, J-
dc.contributor.authorBland-Hawthorn, J-
dc.contributor.authorCampbell, R-
dc.contributor.authorFreeman, KC-
dc.contributor.authorGibson, B-
dc.contributor.authorGilmore, G-
dc.contributor.authorGrebel, EK-
dc.contributor.authorHelmi, A-
dc.contributor.authorMunari, U-
dc.contributor.authorNavarro, JF-
dc.contributor.authorParker, QA-
dc.contributor.authorSeabroke, G-
dc.contributor.authorSiebert, A-
dc.contributor.authorSiviero, A-
dc.contributor.authorWilliams, M-
dc.contributor.authorWyse, RFG-
dc.contributor.authorCombes, F-
dc.contributor.authorSamadi, R-
dc.contributor.editorCharbonnel, C-
dc.date.accessioned2015-07-08T03:23:42Z-
dc.date.available2015-07-08T03:23:42Z-
dc.date.issued2008-
dc.identifier.citationSF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Paris, France, 30 June - 4 July 2008, p. 47-47-
dc.identifier.urihttp://hdl.handle.net/10722/211250-
dc.description.abstractRAVE data has provided new results on Galactic kinematics like the kinematical decomposition of the Galactic disk. This decomposition permits to identify the different components of the disk and to characterize them in terms of scale height and scale length. With the data provided by Gaia and in particular the RVS, we will have a completly renewed view of the Galaxy. The precision of the RVS will permit to undertake a precise analysis of the kinematics of the Galactic disks. This knowledge will provide significant clues to constrain the scenarios of the Galactic disk formation.-
dc.languageeng-
dc.relation.ispartofSF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics-
dc.titleGalactic kinematics from RAVE to Gaia-RVS Data-
dc.typeConference_Paper-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.spage47-
dc.identifier.epage47-

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