A Hubble Space Telescope WFPC2 Investigation of the Nuclear Morphology in the Toomre Sequence of Merging Galaxies
Atomic and Molecular Gas in Colliding Galaxy Systems. I. The Data
Mapping Infrared Enhancements in Closely Interacting Spiral-Spiral Pairs. I. ISO CAM and ISO SWS Observations
Massive Star Clusters in Ongoing Galaxy Interactions: Clues to Cluster Formation
The Toomre Sequence Revisited with HST NICMOS: Nuclear Brightness Profiles and Colors of Interacting and Merging Galaxies
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-03-14T18:14:13Z/1999-03-15T16:17:53Z
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, KEEL WILLIAM C., 2000, 'Do Massive Star Clusters Form in Young and Weak Galaxy Interactions?', 1.0, European Space Agency, https://doi.org/10.5270/esa-jakzm7i