A new ultraluminous X-ray source in the galaxy NGC 5907
HUBBLE SPACE TELESCOPE Imaging of Globular Clusters in the Edge-on Spiral Galaxies NGC 4565 and NGC 5907
Hubble Space Telescope observations of globular cluster systems along the Hubble sequence of spiral galaxies
Low Radiative Efficiency Accretion at Work in Active Galactic Nuclei: The Nuclear Spectral Energy Distribution of NGC 4565
Optical Counterparts of Ultraluminous X-Ray Sources Identified from Archival HST WFPC2 Images
Searching for the Donor Stars of ULX Pulsars
The most extreme ultraluminous X-ray sources: evidence for intermediate-mass black holes?
The Nature of Ultraluminous X-Ray Sources in NGC 4565
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-02-22T20:11:15Z/1996-03-31T23:16:56Z
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, Ashman comma Keith M., 1997, 'DISK GLOBULAR CLUSTERS IN EDGE-ON SPIRAL GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-9mi9kr4