Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1

J. K. Zhao; G. Zhao; W. Aoki; M. N. Ishigaki; T. Suda; T. Matsuno; J. R. Shi; Q. F. Xing; Y. Q. Chen; Terry D. Oswalt; X. M. Kong; X. L. Liang

doi:10.3847/1538-4357/AAE712

Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1

J. K. Zhao
, G. Zhao
, W. Aoki
, M. N. Ishigaki
, T. Suda
, T. Matsuno
, J. R. Shi
, Q. F. Xing
, Y. Q. Chen
, Terry D. Oswalt
, X. M. Kong
, X. L. Liang

Chinese Academy of Sciences
Graduate University for Advanced Studies
Institute for the Physics and Mathematics of the Universe
University of Tokyo
Embry-Riddle Aeronautical University

Research output: Contribution to journal › Article › peer-review

Original language	American English
Journal	The Astrophysical Journal
Volume	868
DOIs	https://doi.org/10.3847/1538-4357/AAE712
State	Published - Nov 27 2018
Externally published	Yes

Disciplines

Astrophysics and Astronomy
Physics

Access to Document

10.3847/1538-4357/AAE712License: Unspecified

Cite this

@article{43cc5d01ea4647208598e1647e116653,

title = "Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1",

author = "Zhao, \{J. K.\} and G. Zhao and W. Aoki and Ishigaki, \{M. N.\} and T. Suda and T. Matsuno and Shi, \{J. R.\} and Xing, \{Q. F.\} and Chen, \{Y. Q.\} and Oswalt, \{Terry D.\} and Kong, \{X. M.\} and Liang, \{X. L.\}",

note = "We present the chemical abundances of six stars in the halo stream Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)-N1, a new kinematically selected substructure from LAMOST data, from high-resolution spectra obtained with the Subaru/High Dispersion Spectrograph. Atmospheric parameters were determined by an iterative procedure based on spectroscopic analysis.",

year = "2018",

month = nov,

day = "27",

doi = "10.3847/1538-4357/AAE712",

language = "American English",

volume = "868",

journal = "The Astrophysical Journal",

issn = "1538-4357",

publisher = "Institute of Physics Publishing, Inc.",

}

TY - JOUR

T1 - Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1

AU - Zhao, J. K.

AU - Zhao, G.

AU - Aoki, W.

AU - Ishigaki, M. N.

AU - Suda, T.

AU - Matsuno, T.

AU - Shi, J. R.

AU - Xing, Q. F.

AU - Chen, Y. Q.

AU - Oswalt, Terry D.

AU - Kong, X. M.

AU - Liang, X. L.

N1 - We present the chemical abundances of six stars in the halo stream Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST)-N1, a new kinematically selected substructure from LAMOST data, from high-resolution spectra obtained with the Subaru/High Dispersion Spectrograph. Atmospheric parameters were determined by an iterative procedure based on spectroscopic analysis.

PY - 2018/11/27

Y1 - 2018/11/27

UR - http://ui.adsabs.harvard.edu/abs/2018ApJ...868..105Z/abstract

U2 - 10.3847/1538-4357/AAE712

DO - 10.3847/1538-4357/AAE712

M3 - Article

SN - 1538-4357

VL - 868

JO - The Astrophysical Journal

JF - The Astrophysical Journal

ER -

Tracing the Origin of Moving Groups. II. Chemical Abundance of Six Stars in the Halo Stream LAMOST-N1

Disciplines

Access to Document

Other files and links

Cite this