Evidence for the strong effect of gas removal on the internal dynamics of young stellar clusters
First direct dynamical detection of a dual supermassive black hole system at sub-kiloparsec separation
From young massive star cluster to old globular: the LV-s0 relationship as a diagnostic tool
Hierarchical star formation in M33: fundamental properties of the star-forming regions
Mass Segregation and the Initial Mass Function of Super Star Cluster M82-F
The impact of satellite trails on Hubble Space Telescope observations
The super star cluster population of the M82 nuclear starburst
Young star clusters in interacting galaxies - NGC 1487 and NGC 4038/4039
Young star clusters in the Antennae galaxies and NGC 1487
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-06-04T00:18:04Z/2003-01-20T07:34:38Z
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, Vacca comma William D., 2004, 'Masses and IMF Variations in Super Star Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-amneey9