Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
A Hubble Space Telescope Survey of the Disk Cluster Population of M31. I. WFPC2 Pointings
A Survey of Star Clusters in the M31 Southwest Field: UBVRI Photometry and Multiband Maps
Determining accurate distances to nearby galaxies
Formation time-scales for high-mass X-ray binaries in M33
M33 X-7: ChASeM33 Reveals the First Eclipsing Black Hole X-Ray Binary
Photometry of Star Clusters in the M 31 Galaxy. Aperture Size Effects
Star Clusters in M33. I. Detection, Morphology, and Photometry
Star Clusters in M33. III. The Youngest Population
Young stellar populations in M33: A comparative HST and GALEX study
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-08-30T22:32:16Z/1995-12-13T14:10:17Z
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, MASSEY PHILIP, 1996, 'THE EVOLUTION OF MASSIVE STARS: CLOSING THE LOOP OBSERVATIONALLY IN THE LOCAL GROUP', 1.0, European Space Agency, https://doi.org/10.5270/esa-0afgf9b