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Vertical velocity patterns in the Milky Way disc: RAVE-Gaia streaming motions

Published online by Cambridge University Press:  02 August 2018

I. Carrillo
Affiliation:
Leibniz Institut für Astrophysik Potsdam (AIP), An der Sterwarte 16, D-14482 Potsdam, Germany email: icarrillo@aip.de
I. Minchev
Affiliation:
Leibniz Institut für Astrophysik Potsdam (AIP), An der Sterwarte 16, D-14482 Potsdam, Germany email: icarrillo@aip.de
G. Kordopatis
Affiliation:
Leibniz Institut für Astrophysik Potsdam (AIP), An der Sterwarte 16, D-14482 Potsdam, Germany email: icarrillo@aip.de Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, 06304, Nice cedex 4, France
M. Steinmetz
Affiliation:
Leibniz Institut für Astrophysik Potsdam (AIP), An der Sterwarte 16, D-14482 Potsdam, Germany email: icarrillo@aip.de
RAVE
Affiliation:
Leibniz Institut für Astrophysik Potsdam (AIP), An der Sterwarte 16, D-14482 Potsdam, Germany email: icarrillo@aip.de Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, 06304, Nice cedex 4, France
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Abstract

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Using data from the Radial Velocity Experiment (RAVE) and the Tycho- Gaia astrometric solution catalogue (TGAS), we study the vertical velocity (Vz) patterns in the Milky Way disc. We search in particular for variation in velocity with distance above and below the disc midplane. In contrast to previous suggestions of a breathing mode seen in RAVE data, our results support a combination of bending and breathing modes, likely generated by a combination of external or internal and external mechanisms.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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