A high-resolution radio study of neutral gas in the starburst galaxy NGC 520
A Hubble Space Telescope WFPC2 Investigation of the Nuclear Morphology in the Toomre Sequence of Merging Galaxies
An X-ray view of 82 LINERs with Chandra and XMM-Newton data
Infrared mergers and infrared quasi-stellar objects with galactic winds - I. NGC 2623: nuclear outflow in a proto-elliptical candidate
Optical Counterparts of Ultraluminous X-Ray Sources Identified from Archival HST WFPC2 Images
Optical spectroscopy of type 2 LINERs
Radio Emission Associated with Ultraluminous X-Ray Sources in the Galaxy Merger NGC 3256
Secondary Radio and X-Ray Emissions from Galaxy Mergers
The nature of nuclear Ha emission in LINERs
The nearest extreme starburst: bubbles, young star clusters and outflow in the merger NGC 3256
The Toomre Sequence Revisited with HST NICMOS: Nuclear Brightness Profiles and Colors of Interacting and Merging Galaxies
X-ray nature of the LINER nuclear sources
Instrument
STIS, STIS/CCD, WFPC2, WFPC2/PC
Temporal Coverage
2000-06-06T18:31:14Z/2003-03-05T20:34:10Z
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, van der Marel comma Roeland P., 2007, 'Merger-driven evolution of galactic nuclei: observations of the Toomre sequence', 1.0, European Space Agency, https://doi.org/10.5270/esa-scqpk9e