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Three Wide Binaries in LAMOST Pilot Survey

Published online by Cambridge University Press:  06 January 2014

J. K. Zhao
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; email: [email protected], [email protected]
G. Zhao
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; email: [email protected], [email protected]
T. D. Oswalt
Affiliation:
Physics and Space Science Department, Florida Institute of Technology, Melbourne, FL 32901, USA email: [email protected]
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Abstract

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Three wide binary candidates that have been identified in the Large sky Area Multi-Object Spectroscopic Telescope (LAMOST) pilot survey data are presented. All three consist of main sequence stars of relatively late spectral type.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Dhital, S., West, A. A., Stassun, K. G., & Bochanski, J. J. 2010, AJ, 139, 2566CrossRefGoogle Scholar
Sesar, B., Ivezić, Z., & Jurić, M. 2008, ApJ, 689, 1244CrossRefGoogle Scholar
Zhao, J. K., Oswalt, T. D., & Zhao, G. 2012, AJ, 143, 31CrossRefGoogle Scholar