Fundamental Properties and Distances of Large Magellanic Cloud Eclipsing Binaries. III. EROS 1044
Fundamental Properties and Distances of Large Magellanic Cloud Eclipsing Binaries. IV. HV 5936
Fundamental Properties and Distances of the Large Magellanic Cloud from Eclipsing Binaries. II. HV 982
Investigation of the Magellanic eclipsing binary HV 2241
The Distance to the Large Magellanic Cloud from the Eclipsing Binary HV 2274
The Large Magellanic Cloud Eclipsing Binary HV 2274: Fundamental Properties and Comparison with Evolutionary Models
Instrument
FOS/BL, HRS/2
Temporal Coverage
1996-09-27T08:19:10Z/1997-01-31T11:51:51Z
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, Guinan comma Edward F., 1998, 'ECLIPSING BINARIES IN THE MAGELLANIC CLOUDS - FUNDAMENTAL PROPERTIES AND DISTANCES', 1.0, European Space Agency, https://doi.org/10.5270/esa-q9azg3i