Kinematic groups beyond the solar neighbourhood with RAVE

T. Antoja*, A. Helmi, O. Bienayme, J. Bland-Hawthorn, B. Famaey, K. Freeman, B. K. Gibson, G. Gilmore, E. K. Grebel, I. Minchev, U. Munari, J. Navarro, Q. Parker, W. Reid, G. M. Seabroke, A. Siebert, A. Siviero, M. Steinmetz, M. Williams, R. WyseT. Zwitter

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

50 Citations (Scopus)

Abstract

We analyse the kinematics of disc stars observed by the RAdial Velocity Experiment (RAVE) survey in and beyond the solar neighbourhood. We detect significant overdensities in the velocity distributions using a technique based on the wavelet transform. We find that the main local kinematic groups are large-scale features, surviving at least up to ~1 kpc from the Sun in the direction of antirotation, and also at ~700 pc below the Galactic plane. We also find that for regions located at different radii than the Sun, the known groups appear shifted in the vR-vφ velocity plane. For example, the Hercules group has a larger azimuthal velocity for regions inside the solar circle and a lower value outside. We have also discovered a newgroup at (U, V) = (92,-22) km s-1 in the solar neighbourhood and confirmed the significance of other previously found groups. Some of these trends detected for the first time are consistent with dynamical models of the effects of the bar and the spiral arms. More modelling is required to definitively characterize the non-axisymmetric components of our Galaxy using these groups.

Original languageEnglish
Pages (from-to)L1-L5
Number of pages5
JournalMonthly Notices of the Royal Astronomical Society: Letters
Volume426
Issue number1
DOIs
Publication statusPublished - Oct 2012

Fingerprint

Dive into the research topics of 'Kinematic groups beyond the solar neighbourhood with RAVE'. Together they form a unique fingerprint.

Cite this