Black holes and core expansion in massive star clusters
Chemical Compositions of Red Giant Stars in Old Large Magellanic Cloud Globular Clusters
Comparing the properties of local globular cluster systems: implications for the formation of the Galactic halo
Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud - III. Horizontal branch morphology
HSTcolour-magnitude diagrams of six old globular clusters in the LMC
New Optical and Near-Infrared Surface Brightness Fluctuation Models. II. Young and Intermediate-Age Stellar Populations
Quantifying Quasar Variability as Part of a General Approach to Classifying Continuously Varying Sources
Star Formation Histories from Hubble Space Telescope Color-Magnitude Diagrams of Six Fields of the Large Magellanic Cloud
Stellar Crowding and the Science Case for Extremely Large Telescopes
Surface brightness profiles and structural parameters for 53 rich stellar clusters in the Large Magellanic Cloud
The Star Formation History of the Large Magellanic Cloud
The VMC survey - XLIII. The spatially resolved star formation history across the Large Magellanic Cloud
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-10-18T05:34:16Z/1995-12-10T04:11:17Z
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, Suntzeff et al., 1996, 'THE OLDEST GLOBULAR CLUSTERS IN THE LARGE MAGELLANIC CLOUD', 1.0, European Space Agency, https://doi.org/10.5270/esa-jc5c2gu
