Extinction in the Large Magellanic Cloud Bar around NGC 1854, NGC 1856, and NGC 1858
Multiple stellar populations in Magellanic Cloud clusters - III. The first evidence of an extended main sequence turn-off in a young cluster: NGC 1856
Multiple stellar populations in Magellanic Cloud clusters - VI. A survey of multiple sequences and Be stars in young clusters
NGC 1856: Using Machine Learning Techniques to Uncover Detailed Stellar Abundances from MUSE Data
The impact of satellite trails on Hubble Space Telescope observations
The Radial Distributions of the Two Main-sequence Components in the Young Massive Star Cluster NGC 1856
The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2014-02-09T08:03:15Z/2014-06-11T19:27:35Z
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, Milone et al., 2015, 'Multiple stellar populations in the young Large Magellanic Cloud cluster NGC1856', 1.0, European Space Agency, https://doi.org/10.5270/esa-deq8s9d