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Closing remarks and Outlook

Published online by Cambridge University Press:  02 August 2018

Francoise Combes Open the ORCID record for Francoise Combes [Opens in a new window]
Francoise Combes*
Affiliation:
Observatoire de Paris, LERMA, College de France, CNRS, PSL, Sorbonne Univ. UPMC, F-75014, Paris, France email: francoise.combes@obspm.fr
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Abstract

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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

Galaxy: abundancesGalaxy: bulgeGalaxy: diskGalaxy: evolutionGalaxy: haloGalaxy: kinematics and dynamicsGalaxy: structurestars: abundances
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S334: Rediscovering our Galaxy , July 2017 , pp. 248 - 255
Copyright
Copyright © International Astronomical Union 2018 

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