Abundant molecular gas in tidal dwarf galaxies: On-going galaxy formation
Accurate positions for the ultraluminous X-ray sources NGC 7319-X4 and NGC 5474-X1 and limiting magnitudes for their optical counterparts
A dichotomy in the orientation of dust and radio jets in nearby low-power radio galaxies
A High-Resolution Mosaic of Molecular Gas in Stephans Quintet
A Multiwavelength Study of Stephans Quintet
Gemini Spectroscopic Survey of Young Star Clusters in Merging/Interacting Galaxies. IV. Stephans Quintet
Hubble Space Telescope Images of Stephans Quintet: Star Cluster Formation in a Compact Group Environment
Molecular and ionized gas in the tidal tail in Stephans Quintet
Observations and modeling of the dust emission from the H2-bright galaxy-wide shock in Stephans Quintet
The Discovery of a High-Redshift X-Ray-Emitting QSO Very Close to the Nucleus of NGC 7319
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1998-12-30T03:36:14Z/1999-06-17T20:24:33Z
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, Charlton et al., 2000, 'Formation of Stellar Systems in Mergers in a Compact Group of Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-1fdi2pw
