Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
Blending of Cepheids in M33
Determination of the Distance to M33 Based on Single-Epoch I-Band Hubble Space Telescope Observations of Cepheids
Determination of the Distance to M33 Based on the Tip of the Red Giant Branch and the Red Clump
Formation time-scales for high-mass X-ray binaries in M33
Hubble Space Telescope WFPC2 Color-Magnitude Diagrams of Halo Globular Clusters in M33: Implications for the Early Formation History of the Local Group
Hubble Space Telescope WFPC2 Photometry of M33: Properties of the Halo Star Clusters and Surrounding Fields
Kinematics of Star Clusters in M33: Distinct Populations
Mass-to-Light Ratios for M31 Globular Clusters: Age Dating and a Surprising Metallicity Trend
Star clusters in M 33. IV. A new survey from deep HST images
Structural Parameters and Dynamical Masses for Globular Clusters in M33
Structural Parameters for 10 Halo Globular Clusters in M33
The Supernova Progenitor Mass Distributions of M31 and M33: Further Evidence for an Upper Mass Limit
Tip of the Red Giant Branch Distances. II. Zero-Point Calibration
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-10-28T12:30:17Z/1997-07-11T23:13:53Z
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, Sarajedini comma Ata, 1998, 'The Formation History of Globular Clusters in M33', 1.0, European Space Agency, https://doi.org/10.5270/esa-8apzk6f