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The Mixed Origin of the Galactic Thick Disk†

Published online by Cambridge University Press:  06 January 2014

W. Y. Cui ,
C. Liu ,
P. de Laverny ,
A. Recio-Blanco  and
G. Van de Ven
W. Y. Cui
Affiliation:
Department of Physics, Shandong University, Jinan, Shandong 250100, China email: wycui@bao.ac.cn Department of Physics, Hebei Normal University, Shijiazhuang, Hebei 050024, China
C. Liu
Affiliation:
National Astronomical observatories, Chinese Academy of Sciences, Beijing 100012, China
P. de Laverny
Affiliation:
Observatoire de la Côte d'Azur, Dpt. Cassiopée UMR6 202, 06 304 Nice Cedex 4, France
A. Recio-Blanco
Affiliation:
Observatoire de la Côte d'Azur, Dpt. Cassiopée UMR6 202, 06 304 Nice Cedex 4, France
G. Van de Ven
Affiliation:
Max-Planck-Institut für Astronomie, Königstuhl 17, D-69117 Heidelberg, Germany
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Abstract

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We found that the thick disk stars of the Galaxy should form from gas-rich mergers and minor merger or radial migration.

Keywords

Galaxyabundancesdiscformationkinematics and dynamics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 402
Copyright
Copyright © International Astronomical Union 2014 

Footnotes

†

This work is supported be NSFC 1100302, U1231119, 11273011, CPSF 2013M531587, NSFH A2011205102, CPRC034.

References

† This work is supported be NSFC 1100302, U1231119, 11273011, CPSF 2013M531587, NSFH A2011205102, CPRC034.