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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, FBinney, JBland-Hawthorn, JCampbell, RFreeman, KGibson, BGilmore, GGrebel, EKHelmi, AMunari, U Navarro, JFParker, QASeabroke, GSiebert, ASiviero, AWilliams, MWyse, RFG
Issue Date1-Jul-2008
Abstract

RAVE 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/10722/342949

 

DC FieldValueLanguage
dc.contributor.authorVeltz, L-
dc.contributor.authorBienaymé, O-
dc.contributor.authorSteinmetz, M-
dc.contributor.authorZwitter, T-
dc.contributor.authorWatson, F-
dc.contributor.authorBinney, J-
dc.contributor.authorBland-Hawthorn, J-
dc.contributor.authorCampbell, R-
dc.contributor.authorFreeman, K-
dc.contributor.authorGibson, B-
dc.contributor.authorGilmore, G-
dc.contributor.authorGrebel, EK-
dc.contributor.authorHelmi, A-
dc.contributor.authorMunari, U Navarro, 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.date.accessioned2024-05-08T02:52:53Z-
dc.date.available2024-05-08T02:52:53Z-
dc.date.issued2008-07-01-
dc.identifier.urihttp://hdl.handle.net/10722/342949-
dc.description.abstract<p>RAVE 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.</p>-
dc.languageeng-
dc.relation.ispartofSF2A-2008: Annual meeting of the French Society of Astronomy and Astrophysics (30/06/2008-04/07/2008)-
dc.titleGalactic kinematics from RAVE to Gaia-RVS Data-
dc.typeConference_Paper-
dc.identifier.volume1-

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