Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S330(12), p. 193-196, 2017
DOI: 10.1017/s1743921317006093
Full text: Unavailable
AbstractThe LAMOST Galactic surveys provide robust stellar atmospheric parameters, abundances, masses and ages of millions of stars, allowing a unprecedented mapping of matter distribution, spatial structure, star formation rate, chemistry and kinematics of the Galaxy. In this proceeding we present structure and metallicity of the Galactic disk revealed by mono-age stellar populations within a few kilo-parsec of the solar neighborhood.