24–29 giu 2018
LNGS
Europe/Rome fuso orario

Dynamical and chemical evolution of the Milky Way from Optical and IR spectroscopic Surveys

26 giu 2018, 17:30
30m
"E. Fermi" conference room (LNGS)

"E. Fermi" conference room

LNGS

Via G. Acitelli, 22 - 67100 Assergi (Italy)

Relatore

Sofia Randich (INAF - OAA)

Descrizione

In the last decade or so a variety of ground based spectroscopic surveys of the Milky Way have been undertaken. These projects are yielding accurate kinematics and abundances for large, statistically significant samples of stars belonging to different Galactic populations. I will review the main results from those surveys, and discuss their huge impact on our understanding of the chemical and dynamical evolution of the Galaxy, as well as on stellar nucleosynthesis.

Autore principale

Sofia Randich (INAF - OAA)

Materiali di presentazione