A far-ultraviolet variability survey of the globular cluster M80
Cataclysmic and Close Binaries in Star Clusters. V. Erupting Dwarf Novae, Faint Blue Stars, X-Ray Sources, and the Classical Nova in the Core of M80
Central dynamics of globular clusters
Extragalactic novae
Reconstructing galaxy histories from globular clusters
Search for Pulsating Stars in the Globular Cluster M 80 from Ground- and Space-based Observations
Surface Brightness Profiles of Galactic Globular Clusters from Hubble Space Telescope Images
Testing Photometric Diagnostics for the Dynamical State and Possible Intermediate-mass Black Hole Presence in Globular Clusters
The ubiquitous nature of the horizontal branch second U-jump. A link with the Blue Hook scenario?
Very Large Array Limits for Intermediate-Mass Black Holes in Three Globular Clusters
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1997-08-29T04:23:13Z/1997-10-03T05:37:33Z
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, Shara comma Michael, 1998, 'Where are the Dozens of Predicted Cataclysmic Variables in Globular Clusters?', 1.0, European Space Agency, https://doi.org/10.5270/esa-k4jvd7p