Blue Straggler Stars beyond the Milky Way. II. A Binary Origin for Blue Straggler Stars in Magellanic Cloud Clusters
Blue Straggler Stars beyond the Milky Way. IV. Radial Distributions and Dynamical Implications
Different Stellar Rotations in the Two Main Sequences of the Young Globular Cluster NGC 1818: The First Direct Spectroscopic Evidence
Hubble Space Telescope survey of Magellanic Cloud star clusters. Photometry and astrometry of 113 clusters and early results
Multiple stellar populations in Magellanic Cloud clusters - VI. A survey of multiple sequences and Be stars in young clusters
Photometric binaries in 14 Magellanic Cloud star clusters
Rotation and Ha Emission in a Young SMC Cluster: A Spectroscopic View of NGC 330
The impact of satellite trails on Hubble Space Telescope observations
The single star path to Be stars
The Spatial Distributions of Blue Main-sequence Stars in Magellanic Cloud Star Clusters
The young massive SMC cluster NGC 330 seen by MUSE. III. Stellar parameters and rotational velocities
The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population
The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content
When Do Stars Go Boom?
Instrument
ACS/WFC, WFC3/UVIS
Temporal Coverage
2016-12-21T21:55:52Z/2017-10-06T20:48:55Z
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., 2018, 'Multiple Stellar Populations in Young Magellanic Cloud Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-gsyfhtr
