Astrometry of the globular cluster 47 Tucanae and possible optical identification of X-ray sources.
Bulges of Nearby Galaxies with Spitzer: The Growth of Pseudobulges in Disk Galaxies and its Connection to Outer Disks
Cataclysmic and Close Binaries in Star Clusters. IV. The Unexpectedly Low Number of Erupting Dwarf Novae Detected by the Hubble Space Telescope in the Core of 47 Tucanae
First Astronomical Images Sharpened with Adaptive Optics Using a Sodium Laser Guide Star
Globular Cluster Photometry With the Hubble Space Telescope. I. Description of the Method and Analysis of the Core of 47 TUC
Globular Cluster Photometry with the Hubble Space Telescope.VI.WF/PC-I Observations of the Stellar Populations in the Core of M13 (NGC 6205)
Instrument
WFPC/PC
Temporal Coverage
1991-01-22T05:51:13Z/1991-04-03T10:39:48Z
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, Bahcall comma John, 1992, 'THE STELLAR DENSITY DISTRIBUTIONS IN THE CENTERS OF GALACTIC GLOBULAR CLUSTERS II. CYCLE 0 MAJOR CHANGES', 1.0, European Space Agency, https://doi.org/10.5270/esa-k0146gf