Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey

A project of a spectroscopic survey of Galactic structure and evolution with a Large sky Area Multi-Object fiber Spectroscopic Telescope （LAMOST） is presented. The spectroscopic survey consists of two observational modes for various targets in our Galaxy. One is a major survey of the Milky Way aimed...

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Bibliographic Details
Published in:Chinese journal of astronomy and astrophysics 2006-06, Vol.6 (3), p.265-280
Main Authors: Zhao, Gang, Chen, Yu-Qin, Shi, Jian-Rong, Liang, Yan-Chun, Hou, Jin-Liang, Chen, Li, Zhang, Hua-Wei, Li, Ai-Gen
Format: Article
Language:English
Subjects:
分光镜
银河天文学
银河系
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Summary:A project of a spectroscopic survey of Galactic structure and evolution with a Large sky Area Multi-Object fiber Spectroscopic Telescope （LAMOST） is presented. The spectroscopic survey consists of two observational modes for various targets in our Galaxy. One is a major survey of the Milky Way aimed at a systematic study of the stellar abundance and Galactic chemical evolution through low resolution （R = 1000 2000） spectroscopy. Another is a follow-up observation with medium resolution （R = 10000） spectrographs aimed at detailed studies of the selected stars with different chemical composition, kinematics and dynamics.
ISSN:1009-9271
DOI:10.1088/1009-9271/6/3/01