Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-10T14:13:50.325Z Has data issue: false hasContentIssue false
  • English
  • Français

Three Wide Binaries in LAMOST Pilot Survey

Published online by Cambridge University Press:  06 January 2014

J. K. Zhao ,
G. Zhao  and
T. D. Oswalt
J. K. Zhao
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; email: zjk@bao.ac.cn, gzhao@bao.ac.cn
G. Zhao
Affiliation:
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China; email: zjk@bao.ac.cn, gzhao@bao.ac.cn
T. D. Oswalt
Affiliation:
Physics and Space Science Department, Florida Institute of Technology, Melbourne, FL 32901, USA email: toswalt@fit.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 456
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