A black hole detected in the young massive LMC cluster NGC 1850
A closer look at the binary content of NGC 1850
Dissecting the extended main-sequence turn-off of the young star cluster NGC 1850
Exploring the role of binarity in the origin of the bimodal rotational velocity distribution in stellar clusters
Hubble Space Telescope survey of Magellanic Cloud star clusters: UV-dim stars in young clusters
Multiple stellar populations in Magellanic Cloud clusters - VI. A survey of multiple sequences and Be stars in young clusters
On the origin of UV-dim stars: a population of rapidly rotating shell stars?
On the precision of full-spectrum fitting of simple stellar populations - IV. A systematic comparison with results from colour-magnitude diagrams
Stars caught in the braking stage in young Magellanic Cloud clusters
The effects of stellar rotation along the main sequence of the 100-Myr-old massive cluster NGC 1850
The impact of satellite trails on Hubble Space Telescope observations
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
2015-10-22T12:32:01Z/2015-10-22T16:01:29Z
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, Goudfrooij et al., 2016, 'Probing Extended Star Formation in the Young Massive Cluster NGC 1850', 1.0, European Space Agency, https://doi.org/10.5270/esa-sbuwa9p
