The wobbly Galaxy: Kinematics north and south with RAVE red-clump giants

M. E K Williams*, M. Steinmetz, J. Binney, A. Siebert, H. Enke, B. Famaey, I. Minchev, R. S. de Jong, C. Boeche, K. C. Freeman, O. Bienaymé, J. Bland-Hawthorn, B. K. Gibson, G. F. Gilmore, E. K. Grebel, A. Helmi, G. Kordopatis, U. Munari, J. F. Navarro, Q. A. ParkerW. Reid, G. M. Seabroke, S. Sharma, A. Siviero, F. G. Watson, R. F G Wyse, T. Zwitter

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    176 Citations (Scopus)
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    TheRAdialVelocity Experiment survey, combined with proper motions and distance estimates, can be used to study in detail stellar kinematics in the extended solar neighbourhood (solar suburb). Using 72 365 red-clump stars, we examine the mean velocity components in 3D between 6 < R < 10 kpc and -2 < Z < 2 kpc, concentrating on north-south differences. Simple parametric fits to the (R, Z) trends for Vφ and the velocity dispersions are presented. We confirm the recently discovered gradient in mean Galactocentric radial velocity, VR, finding that the gradient is marked below the plane (δ(VR)/δR=-8 kms-1 kpc-1 for Z<0, vanishing to zero above the plane), with a Z gradient thus also present. The vertical velocity, VZ, also shows clear, large-amplitude (|VZ| = 17 km s-1) structure, with indications of a rarefaction- compression pattern, suggestive of wave-like behaviour. We perform a rigorous error analysis, tracing sources of both systematic and random errors. We confirm the north-south differences in VR and VZ along the line of sight, with the VR estimated independent of the proper motions. The complex three-dimensional structure of velocity space presents challenges for future modelling of the Galactic disc, with the Galactic bar, spiral arms and excitation of wave-like structures all probably playing a role.

    Original languageEnglish
    Pages (from-to)101-121
    Number of pages21
    JournalMonthly Notices of the Royal Astronomical Society
    Issue number1
    Publication statusPublished - Nov 2013

    Bibliographical note

    This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. Copyright 2013 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.


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