2D kinematics of massive stars near the Galactic Centre
A first glimpse at the line-of-sight structure of the Milky Ways nuclear stellar disc
Co-moving groups around massive stars in the nuclear stellar disk
HST Astrometry in the 30 Doradus Region. II. Runaway Stars from New Proper Motions in the Large Magellanic Cloud
Mapping the core of the Tarantula Nebula with VLT-MUSE - III. A template for metal-poor starburst regions in the visual and far-ultraviolet
Spectroscopic evidence of a possible young stellar cluster at the Galactic Center
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2012-10-01T03:08:54Z/2012-10-07T08:21:10Z
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, Lennon comma Daniel J., 2013, 'PROPER MOTIONS OF ISOLATED MASSIVE STARS NEAR THE GALACTIC CENTER', 1.0, European Space Agency, https://doi.org/10.5270/esa-yv82fte