Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey

Details Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjaa...6..265z&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Volume 6, Issue 3, pp. 265-280 (2006).

Astronomy and Astrophysics

Astrophysics

18

Scientific paper

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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