New Optical and Near-Infrared Surface Brightness Fluctuation Models. II. Young and Intermediate-Age Stellar Populations
Pulsational Evidence for Mass Loss in NGC 1866 Cepheids
The Distance of the Large Magellanic Cloud Cluster NGC 1866
The Distance to the Large Magellanic Cloud Cluster NGC 1866 and the Surrounding Field
The Luminosity Function of the Large Magellanic Cloud Globular Cluster NGC 1866
The Star-Formation History in the Vicinity of NGC 1866 in the Large Magellanic Cloud
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-10-18T11:18:13Z/1999-10-19T16:27:03Z
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, Walker comma Alistair, 2000, 'NGC 1866: A Critical test of Stellar Evolution for Intermediate Mass Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-za2ogr8