Black holes and core expansion in massive star clusters
Constraining globular cluster formation through studies of young massive clusters - III. A lack of gas and dust in massive stellar clusters in the LMC and SMC
Determination of the IMF in the LMC Stellar Cluster NGC 2156
Discovery of Extended Main-sequence Turnoffs in Four Young Massive Clusters in the Magellanic Clouds
HST WFPC2 Observations of the Peculiar Main Sequence of the Double Star Cluster NGC 2011 in the Large Magellanic Cloud
Pulsational Evidence for Mass Loss in NGC 1866 Cepheids
Surface brightness profiles and structural parameters for 53 rich stellar clusters in the Large Magellanic Cloud
The Initial Mass Function toward the Low-Mass End in the Large Magellanic Cloud with Hubble Space Telescope WFPC2 Observations
The Low End of the Initial Mass Function in Young Clusters. II. Evidence for Primordial Mass Segregation in NGC 330 in the Small Magellanic Cloud
The Low-Mass Pre-Main-Sequence Population of the Stellar Association LH 52 in the Large Magellanic Cloud Discovered with Hubble Space Telescope WFPC2 Observations
When Do Stars Go Boom?
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-08-01T20:19:13Z/2000-09-16T01:45:03Z
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, Nota et al., 2001, 'Is the IMF universal at low stellar masses?', 1.0, European Space Agency, https://doi.org/10.5270/esa-u4p0kqd
