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

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

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@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",

}

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

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

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