A Chandra X-Ray Study of the Interacting Binaries in the Old Open Cluster NGC 6791
Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. II. Age dependencies and new insights
Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. I. Measurements, methods, and first results
A white dwarf cooling age of 8Gyr for NGC 6791 from physical separation processes
Color-Magnitude Diagrams and Luminosity Functions Down to the Hydrogen-Burning Limit. III. A Preliminary Hubble Space Telescope Study of NGC 6791
Reaching the End of the White Dwarf Cooling Sequence in NGC 6791
Survey of Multiple Populations in Globular Clusters among Very-low-mass Stars
The absolute motion of the peculiar cluster NGC 6791
The impact of satellite trails on Hubble Space Telescope observations
The Puzzling White Dwarf Cooling Sequence in NGC 6791: A Simple Solution
The White Dwarf Cooling Sequence in NGC 6791
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2003-07-16T07:45:15Z/2003-07-17T13:03:27Z
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, King comma Ivan R., 2004, 'The Bottom of the Main Sequence in the Old, Metal-Rich Cluster, NGC 6791', 1.0, European Space Agency, https://doi.org/10.5270/esa-nqh26di