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Constraining the Milky Way non-axisymmetries with Gaia

Published online by Cambridge University Press:  14 May 2020

B. Famaey Open the ORCID record for B. Famaey [Opens in a new window] ,
G. Monari ,
A. Siebert ,
O. Bienaymé ,
R. Ibata ,
C. Wegg  and
O. Gerhard
B. Famaey
Affiliation:
Université de Strasbourg, CNRS UMR 7550, Observatoire astronomique de Strasbourg email: [email protected]
G. Monari
Affiliation:
Université de Strasbourg, CNRS UMR 7550, Observatoire astronomique de Strasbourg email: [email protected]
A. Siebert
Affiliation:
Université de Strasbourg, CNRS UMR 7550, Observatoire astronomique de Strasbourg email: [email protected]
O. Bienaymé
Affiliation:
Université de Strasbourg, CNRS UMR 7550, Observatoire astronomique de Strasbourg email: [email protected]
R. Ibata
Affiliation:
Université de Strasbourg, CNRS UMR 7550, Observatoire astronomique de Strasbourg email: [email protected]
C. Wegg
Affiliation:
Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire Lagrange
O. Gerhard
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Garching
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Abstract

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The unprecedented amount and accuracy of kinematic data from the second release of the Gaia mission have started revolutionizing our understanding of the dynamics of the Milky Way disk. The detailed stellar velocity field in the Galactic disk should allow us to constrain with unprecedented precision the parameters of the non-axisymmetric modes of the disk. We present here the status of our current modelling efforts in this area, and their implication on the dynamics of the Galactic bar in particular.

Keywords

Galaxy: kinematics and dynamicsGalaxy: diskGalaxy: structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 61 - 64
Copyright
© International Astronomical Union 2020

References

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