Closing remarks and Outlook
Abstract
Some highlights are given of the IAU Symposium 334, Rediscovering our Galaxy, held in Potsdam, in July 2017: from the first stars fossil records found in the halo, the carbon-enhanced metal poor CEMP-no, to the cosmological simulations presenting possible scenarios for the Milky Way formation, passing through the chemo-dynamical models of the various components, thin and thick disks, box/peanut bulge, halo, etc. The domain is experiencing (or will be in the near future) huge improvements with precise and accurate stellar ages, provided by astero-seismology, precise stellar distances and kinematics (parallaxes and proper motions from GAIA), and the big data resulting from large surveys are treated with deep learning algorithms.
Keywords
Cite
@article{arxiv.1707.07602,
title = {Closing remarks and Outlook},
author = {F. Combes},
journal= {arXiv preprint arXiv:1707.07602},
year = {2018}
}
Comments
8 pages, no figure, in "Rediscovering our Galaxy",Proceedings IAU Symposium No. 334, 2017, C. Chiappini, I. Minchev, E. Starkenburg, M. Valentini., eds