Intermediate and old age Open Clusters science case for high resolution spectroscopy

Bibcode
2017hsa9.conf..508J
Jordi, C.; Carrera, R.; Balaguer-Núnez, L.; Casamiquela, L.
Bibliographical reference

Highlights on Spanish Astrophysics IX, Proceedings of the XII Scientific Meeting of the Spanish Astronomical Society held on July 18-22, 2016, in Bilbao, Spain, ISBN 978-84-606-8760-3. S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernández-Monteagudo, A. Sánchez-Lavega, S. Pérez-Hoyos (eds.), 2017 , p. 508-508

Advertised on:
3
2017
Number of authors
4
IAC number of authors
1
Citations
0
Refereed citations
0
Description
Open Clusters are dynamically-bound groups of stars that formed from the same giant molecular cloud, having a similar age and bulk chemical composition. Open Clusters are key objects for studying the formation and evolution of the Galactic disk. They are targets in on-going large spectroscopic surveys like Gaia-ESO and OCCASO surveys. We discuss the science case of the intermediate age and old Open Clusters for WEAVE, the upcoming multifiber spectroscopic facility in the WHT. In particular we do an overview of the target selection and the survey strategy. Additionally, the impact of the discovery of new clusters by Gaia space mission is discussed.
Type
Non-refereed

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