Blue Straggler Stars beyond the Milky Way. II. A Binary Origin for Blue Straggler Stars in Magellanic Cloud Clusters
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud - III. Horizontal branch morphology
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud - II. Relative ages and distances for six ancient globular clusters
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud - IV. Evidence for multiple populations in Hodge 11 and NGC 2210
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud - V. Multiple populations in ancient globular clusters
Multiple Stellar Populations at Less Evolved Stages. III. A Possible Helium Spread in NGC 2210
Size diversity of old Large Magellanic Cloud clusters as determined by internal dynamical evolution
Star-density Profiles of Six Old Star Clusters in the Large Magellanic Cloud
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2015-12-10T06:36:43Z/2017-04-20T23:27:41Z
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, Sarajedini et al., 2018, 'Exploring the nature and synchronicity of early cluster formation in the Local Group', 1.0, European Space Agency, https://doi.org/10.5270/esa-i42p65v