Ages of M33 Star Clusters Based on the Hubble Space Telescope/WFPC2 Photometry
An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations
A Possible High Nova Rate for Two Local Group Dwarf Galaxies: M32 and NGC 205
A SAURON study of M32: measuring the intrinsic flattening and the central black hole mass
A Slowly Precessing Disk in the Nucleus of M31 as the Feeding Mechanism for a Central Starburst
A Strong Correlation between Circumnuclear Dust and Black Hole Accretion in Early-Type Galaxies
Blending of Cepheids in M33
Blue Horizontal-Branch Stars in Old, Metal-rich Stellar Systems
Distance to M31 with the Hubble Space Telescope and HIPPARCOS Red Clump Stars
Dynamical Correlations for Globular Clusters in M31,
Efficient multi-Gaussian expansion of galaxies
Formation time-scales for high-mass X-ray binaries in M33
Gas Accretion in the M32 Nucleus: Past and Present
High Spatial Resolution Near-Infrared Imaging of the Central Regions of M31
Hubble Space Telescope analysis of stellar populations within the globular cluster G1 (Mayall II) in M 31
Keck Spectroscopy of Red Giant Stars in the Vicinity of M31S Massive Globular Cluster G1
Kinematics of Star Clusters in M33: Distinct Populations
Local Group Populations With the Hubble Space Telescope. I. The M31 Globular Cluster G1=Mayall II
Localization of the X-ray source in the globular cluster G1 with Chandra
M31 Globular Clusters in the Hubble Space Telescope Archive. I. Cluster Detection and Completeness
M31 Globular Clusters in the Hubble Space Telescope Archive. II. Structural Parameters
M31s Heavy-Element Distribution and Outer Disk
M31s Undisturbed Thin Disk of Globular Clusters
Mayall II=G1 in M31: Giant Globular Cluster or Core of a Dwarf Elliptical Galaxy?
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Probing the Nature of the G1 Clump Stellar Overdensity in the Outskirts of M31
Star clusters in M 33. IV. A new survey from deep HST images
Supersoft X-Ray Sources in M31. I. A Chandra Survey and an Extension to Quasi-soft Sources
The Compact UV Nucleus of M33
The Dusty Starburst Nucleus of M33
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-07-29T16:04:16Z/1994-12-29T10:44:17Z
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, Rich comma R. Michael, 1996, 'A STUDY OF THE AGB IN LOCAL GROUP BULGE POPULATIONS', 1.0, European Space Agency, https://doi.org/10.5270/esa-06bpu03