Kinematics of young star clusters with the Gaia-ESO Survey
Date Issued
2017
Author(s)
Abstract
Studying the kinematical properties of young star clusters and star forming regions may help to understand the physical mechanisms driving their dynamical evolution and dissipation into the field. However, due to the lack of high quality data this kind of studies has been carried out only for a small sample of regions. The scenario is rapidly changing thanks to the Gaia-ESO Survey that is observing high resolution spectra of a large sample of clusters in the 1 to 100 Myr age range. In this proceeding we summarize the first results of this project in the field of cluster kinematics.
Volume
88
Start page
660
Issn Identifier
0037-8720
Ads BibCode
2017MmSAI..88..660S
Rights
open.access
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