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Proceedings

What we learn from TGAS about the moving groups of the Solar neighbourhood

MPS-Authors

Goldman,  B.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Schilbach,  E.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Röser,  S.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Schöfer,  P.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Derekas,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Moor,  A.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Brandner,  W.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Henning,  T.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018IAUS..330..214G
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Citation

Goldman, B., Schilbach, E., Röser, S., Schöfer, P., Derekas, A., Moor, A., et al. (2018). What we learn from TGAS about the moving groups of the Solar neighbourhood.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CD90-1
Abstract
We use the TGAS proper motions and parallaxes as well as published and new radial velocities to study the dynamics of nearby moving groups. In particular we try to determine their age using backtracing of the individual members to a common origin. We find that the current data, probably the radial velocities, do not allow to reach a successful conclusion.