Black holes and core expansion in massive star clusters
Comparing the properties of local globular cluster systems: implications for the formation of the Galactic halo
Dynamical masses and mass-to-light ratios of resolved massive star clusters - II. Results for 26 star clusters in the Magellanic Clouds
Hubble Space Telescope Observations of the Oldest Star Clusters in the Large Magellanic Cloud
Surface brightness profiles and structural parameters for 53 rich stellar clusters in the Large Magellanic Cloud
Variable Stars in Large Magellanic Cloud Globular Clusters. I. NGC 1466
Variable Stars in the Large Magellanic Cloud Globular Cluster NGC 2257. I. Results Based on 2007-2008 B, V Photometry
Variable Stars in the LMC Globular Cluster NGC 2257 New: Results Based on 2007-08 B, V Photometry
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-10-13T20:41:17Z/1995-12-13T06:55:57Z
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, Bolte comma Michael, 1996, 'AGES FOR THE OLDEST STAR CLUSTERS IN THE LARGE MAGELLANIC CLOUD', 1.0, European Space Agency, https://doi.org/10.5270/esa-pqzlgof