Journal
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
Volume 6, Issue 3, Pages 265-280Publisher
SCIENCE PRESS
DOI: 10.1088/1009-9271/6/3/01
Keywords
techniques : spectroscopic; stars : abundances; Galaxy : structure; Galaxy : abundances; Galaxy : kinematics and dynamics; Galaxy : evolution
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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.
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