Central K-band kinematics and line strength maps of NGC 1399
Chandra Limits on X-Ray Emission Associated with the Supermassive Black Holes in Three Giant Elliptical Galaxies
Low-Mass X-Ray Binaries in Six Elliptical Galaxies: Connection to Globular Clusters
Measuring Sizes of Marginally Resolved Young Globular Clusters with the Hubble Space Telescope
Molecular disks in radio galaxies. The pathway to ALMA
Optical Counterparts of Ultraluminous X-Ray Sources Identified from Archival HST WFPC2 Images
Recoiling Supermassive Black Holes: A Search in the Nearby Universe
Sizing up Partially Depleted Galaxy Cores
Surface brightness profile reconstruction for elliptical galaxies: the case of Fornax A (NGC 1316)
The Black Hole Mass and Extreme Orbital Structure in NGC 1399
UV/Optical Nuclear Activity in the gE Galaxy NGC 1399
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2000-03-22T09:58:14Z/2000-05-18T06:26:34Z
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, Grillmair comma Carl, 2001, 'The Evolution of Globular Cluster Systems In Early-Type Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-2tx2bv4