A Far-Ultraviolet Survey of 47 Tucanae. II. The Long-Period Cataclysmic Variable AKO 9
Cataclysmic and Close Binaries in Star Clusters. IV. The Unexpectedly Low Number of Erupting Dwarf Novae Detected by the Hubble Space Telescope in the Core of 47 Tucanae
K Giants in 47 Tucanae: Detection of a New Class of Variable Stars
Oscillating Blue Stragglers in the Core of 47 Tucanae
Resolving the Controversy over the Core Radius of 47 Tucanae (NGC 104)
Stellar Variability in the Central Populations of 47 Tucanae from WF/PC Observations with the Hubble Space Telescope. II. Binary Systems
Stellar Variability in the Central Populations of 47 Tucanae from WF/PC Observations with the Hubble Space Telescope. I. Project Overview, Reduction Techniques, and First Results
The Density Profile of 47 Tucanae
Instrument
WFPC/PC
Temporal Coverage
1993-09-04T19:26:16Z/1993-09-06T13:01:16Z
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, Gilliland comma Ronald L, 1994, 'ASTROPHYSICAL STUDY OF BLUE STRAGGLERS IN 47 TUCANAE: CYCLE 3 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-xzvcs2u
