Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S330(12), p. 193-196, 2017

DOI: 10.1017/s1743921317006093

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Galactic Disk Structure and Metallicity from Mono-age Stellar Populations of LAMOST

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

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.

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