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A spectroscopic survey of the Thick Disc outside the Solarneighbourhood: A comparison with the Besançon model

Published online by Cambridge University Press:  15 February 2011

C. Turon ,
F. Meynadier ,
F. Arenou ,
G. Kordopatis ,
A. Recio-Blanco ,
P. de Laverny ,
G. Gilmore ,
V. Hill ,
R.F.G. Wyse  and
A. Helmi
...Show all authors
G. Kordopatis
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
A. Recio-Blanco
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
P. de Laverny
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
G. Gilmore
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
V. Hill
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
R.F.G. Wyse
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
A. Helmi
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
A. Bijaoui
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
C. Ordenovic
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
M. Zoccali
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
O. Bienaymé
Affiliation:
Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Cassiopée, France. e-mail: [email protected]
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Abstract

A spectroscopic survey of nearly 700 stars probing the Galactic Thick Disc far from theSolar neighbourhood is performed. The MATISSE (MATrix Inversion for Spectral SynthEsis)algorithm is developed and trained in order to automatically obtain atmospheric parametersof stars. The derived effective temperatures, surface gravities and overall metallicitiesare then combined to stellar evolution isochrones, radial velocities and proper motions toderive the distances, kinematics and orbital parameters of the sample stars. Results arecompared with simulations from the Besançon model of the Milky Way.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 45: GAIA: At the Frontiers of Astrometry , 2010 , pp. 405 - 408
Copyright
© EAS, EDP Sciences 2011

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References

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