A Multimass Velocity Dispersion Model of 47 Tucanae Indicates No Evidence for an Intermediate-mass Black Hole
A stellar census in globular clusters with MUSE: The contribution of rotation to cluster dynamics studied with 200 000 stars
Constraining Neutrino Cooling Using the Hot White Dwarf Luminosity Function in the Globular Cluster 47 Tucanae
Constraining White Dwarf Structure and Neutrino Physics in 47 Tucanae
Deep HST Imaging in 47 Tucanae: A Global Dynamical Model
Dynamical Estimate of Post-main-sequence Stellar Masses in 47 Tucanae
Formation and Evolution of Blue Stragglers in 47 Tucanae
Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. V. The Rapid Rotation of 47 Tuc Traced and Modeled in Three Dimensions
Long-term observations of the pulsars in 47 Tucanae - I. A study of four elusive binary systems
Outliers: multicolour photometry guiding the search for evolved binary systems in the globular cluster 47 Tucanae
Stellar collisions in globular clusters: Constraints on the initial mass function of the first generation of stars
The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters - IX. The Atlas of multiple stellar populations
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. VIII. Preliminary Public Catalog Release
The Hubble Space Telescope UV legacy survey of galactic globular clusters - XVI. The helium abundance of multiple populations
The impact of satellite trails on Hubble Space Telescope observations
The merger of hard binaries in globular clusters as the primary channel for the formation of second-generation stars
When do stars in 47 Tucanae lose their mass?
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2012-11-14T09:18:29Z/2013-09-20T10:09:19Z
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, Richer comma Harvey B., 2014, 'Completing the Empirical White Dwarf Cooling Sequence: Hot White Dwarfs in 47 Tucanae', 1.0, European Space Agency, https://doi.org/10.5270/esa-h3z7umy