Stellar clusters in the Gaia era
arXiv:1707.01405 · doi:10.1017/S1743921317005294
Abstract
Stellar clusters are important for astrophysics in many ways, for instance as optimal tracers of the Galactic populations to which they belong or as one of the best test bench for stellar evolutionary models. Gaia DR1, with TGAS, is just skimming the wealth of exquisite information we are expecting from the more advanced catalogues, but already offers good opportunities and indicates the vast potentialities. Gaia results can be efficiently complemented by ground-based data, in particular by large spectroscopic and photometric surveys. Examples of some scientific results of the Gaia-ESO survey are presented, as a teaser for what will be possible once advanced Gaia releases and ground-based data will be combined.
8 pages, 8 composite figures, uses pdflatex. To appear in the Proceedings of IAU Symp. 330 (Astrometry and Astrophysics in the Gaia Sky)
References in corpus (12)
- The GALAH Survey: Observational Overview and Gaia DR1 companion
- Exploring Anticorrelations and Light Element Variations in Northern Globular Clusters Observed by the APOGEE Survey
- A VLBI Resolution of the Pleiades Distance Controversy
- APOGEE Chemical Abundances of Globular Cluster Giants in the Inner Galaxy
- Sodium and Oxygen Abundances in the Open Cluster NGC 6791 from APOGEE H-Band Spectroscopy
- Gaia 1 and 2. A pair of new Galactic star clusters
- Two Groups of Red Giants with Distinct Chemical Abundances in the Bulge Globular Cluster NGC 6553 Through the Eyes of APOGEE
- Globular clusters with Gaia
- Highly dynamically evolved intermediate-age open clusters
- Tycho-Gaia Astrometric Solution Parallaxes and Proper Motions for Five Galactic Globular Clusters
- The chemical composition of the stellar cluster Gaia1: no surprise behind Sirius
- , a newly identified intermediate-age Milky Way stellar cluster: A spectroscopic study of 1