Internal dynamics of multiple populations in 28 Galactic globular clusters: a wide-field study with Gaia and the Hubble Space Telescope
Linking photometry and spectroscopy: profiling multiple populations in globular clusters
New Perspective on the Multiple-population Phenomenon in Galactic Globular Clusters from a Wide-field Photometric Survey
Stellar collisions in globular clusters: Constraints on the initial mass function of the first generation of stars
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters - IV. Helium content and relative age of multiple stellar populations within NGC 6352
The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters - IX. The Atlas of multiple stellar populations
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. VIII. Preliminary Public Catalog Release
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. XVIII. Proper-motion Kinematics of Multiple Stellar Populations in the Core Regions of NGC 6352
The Hubble Space Telescope UV legacy survey of galactic globular clusters - XVI. The helium abundance of multiple populations
The impact of satellite trails on Hubble Space Telescope observations
The merger of hard binaries in globular clusters as the primary channel for the formation of second-generation stars
Tracing oCentauris origins: Spatial and chemical signatures of its formation history
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2011-10-31T13:03:31Z/2012-02-14T00:33:59Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Kong et al., 2013, 'Close binary populations in metal-rich globular clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-3zhi8tc