A Color-Magnitude Diagram for a Globular Cluster in the Giant Elliptical Galaxy NGC 5128
A Relation between Supermassive Black Hole Mass and Quasar Metallicity?
Emission Line Properties of Active Galactic Nuclei from a Post-COSTAR Hubble Space Telescope Faint Object Spectrograph Spectral Atlas
Infrared Surface Brightness Fluctuations of the Coma Elliptical Galaxy NGC 4874 and the Value of the Hubble Constant
The Globular Cluster Systems in the Coma Ellipticals. II. Metallicity Distribution and Radial Structure in NGC 4874 and Implications for Galaxy Formation
The Globular Cluster Systems in the Coma Ellipticals. I. The Luminosity Function in NGC 4874 and Implications for Hubbles Constant
The Metallicity Distribution in the Halo Stars of NGC 5128: Implications for Galaxy Formation
The outermost stellar halo of NGC 5128 (Centaurus A): Radial structure
The resolved red giant branches of E/S0 galaxies
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1997-08-16T06:32:13Z/1997-08-24T10:21:53Z
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, Harris comma Gretchen L. H., 1998, 'The Stellar Halo Metallicity Distribution of the Giant Elliptical NGC 5128', 1.0, European Space Agency, https://doi.org/10.5270/esa-wgunsb0