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Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1
The Astrophysical Journal (2018)
  • J. K. Zhao, Chinese Academy of Sciences
  • G. Zhao, Chinese Academy of Sciences
  • W. Aoki, Graduate University for Advanced Studies
  • M. N. Ishigaki, Institute for the Physics and Mathematics of the Universe
  • T. Suda, University of Tokyo
  • T. Matsuno, Graduate University for Advanced Studies
  • J. R. Shi, Chinese Academy of Sciences
  • Q. F. Xing, Chinese Academy of Sciences
  • Y. Q. Chen, Chinese Academy of Sciences
  • Terry D. Oswalt, Embry–Riddle Aeronautical University
  • X. M. Kong, Chinese Academy of Sciences
  • X. L. Liang, Chinese Academy of Sciences
Publication Date
November 27, 2018
DOI
10.3847/1538-4357/AAE712
Citation Information
J. K. Zhao, G. Zhao, W. Aoki, M. N. Ishigaki, et al.. "Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1" The Astrophysical Journal Vol. 868 Iss. 2 (2018) p. 105
Available at: http://works.bepress.com/terry_d_oswalt/105/