A far-ultraviolet variable with an 18-minute period in the globular cluster NGC 1851
A Search for Black Hole Microlensing Signatures in Globular Cluster NGC 6656 (M22)
BSS populations from the WFPC2 UV Survey
Chemical Abundances and Dust in the Halo Planetary Nebula K648 in M15: Its Origin and Evolution Based on an Analysis of Multiwavelength Data
Constraining the True Nature of an Exotic Binary in the Core of NGC 6624
Dynamical age differences among coeval star clusters as revealed by blue stragglers
Hubble Space Telescope Reveals Multiple Sub-giant Branch in Eight Globular Clusters
Old stellar systems in UV: resolved and integrated properties
Proper motions in globular clusters using deconvolution of HST images
Refining the Dynamical Clock for Star Clusters
The blue straggler star population in NGC 6229
The Globular Cluster NGC 6402 (M14). II. Variable Stars
The Optical Counterpart to the X-Ray Transient IGR J1824-24525 in the Globular Cluster M28
The Temperature Distribution of Horizontal Branch Stars: Methods and First Results
The Unimodal Distribution of Blue Straggler Stars in M75 (NGC 6864)
The WFPC2 Ultraviolet Survey: The Blue Straggler Population in NGC 5824
WFPC2 UV survey of Galactic globular clusters. The Horizontal Branch temperature distribution
Instrument
ACS/SBC, WFPC2, WFPC2/PC
Temporal Coverage
2009-03-05T10:28:12Z/2009-05-08T21:21:51Z
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, Ferraro comma Francesco R., 2009, 'UV light from old stellar populations: a census of UV sources in Galactic Globular Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-qz1do7g