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LAMOST Open Clusters Survey: Current Status and Perspective

Published online by Cambridge University Press:  17 July 2015

J.L. Hou ,
L. Chen ,
J. Zhong  and
Z.Y. Shao
J.L. Hou
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, China
L. Chen
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, China
J. Zhong
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, China
Z.Y. Shao
Affiliation:
Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai, China
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Abstract

We have proposed a low Galactic latitude disk survey plan concentrating on open clusters (Chen, Hou et al. 2012) in the LAMOST main survey. We expect to cover more than 400 open clusters in the low Galactic latitude region, and obtain stellar radial velocities as well as abundance information for stars faint as r=16 mag in the cluster fields.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 68: The Milky Way Unravelled by Gaia: GREAT Science from the Gaia Data Releases , 2014 , pp. 377
Copyright
© EAS, EDP Sciences, 2015

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References

Chen, L., Hou, J.L., et al., 2012, RAA, 12, 805
Kharchenko, , et al., 2013, A&A, 558, 53