An X-ray view of 82 LINERs with Chandra and XMM-Newton data
NGC 6240: extended CO structures and their association with shocked gas
Chandra HRC and HST observations of NGC 6240: resolving the active galactic nucleus and starburst
Circumnuclear Star Clusters in the Galaxy Merger NGC 6240, Observed with Keck Adaptive Optics and the Hubble Space Telescope
Discovery of a Binary Active Galactic Nucleus in the Ultraluminous Infrared Galaxy NGC 6240 Using Chandra
Examining the Seyfert-Starburst Connection with Arcsecond-Resolution Radio Continuum Observations
Fast and Furious: Shock Heated Gas as the Origin of Spatially Resolved Hard X-Ray Emission in the Central 5 kpc of the Galaxy Merger NGC 6240
Hubble Space Telescope Observations of NGC 6240: A Case Study of an Ultraluminous Infrared Galaxy with Obscured Activity
Locating the Two Black Holes in NGC 6240
NGC 6240: merger-induced star formation and gas dynamics
Nuclear star formation in NGC 6240
On the formation of star clusters in the merger NGC 6240
Star Formation in Extreme Environments
The Core of NGC 6240 from Keck Adaptive Optics and Hubble Space Telescope NICMOS Observations
The Structure of Active Merger Remnant NGC 6240 from IRAC Observations
Three-Dimensional Integral Field Observations of 10 Galactic Winds. I. Extended Phase (gsim10 Myr) of Mass/Energy Injection Before the Wind Blows
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1999-03-28T16:00:13Z/1999-03-28T21:34:33Z
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, van der Marel et al., 2000, 'Nuclear structure & merger-starburst relation in the ultraluminous IRAS galaxy NGC 6240', 1.0, European Space Agency, https://doi.org/10.5270/esa-f8eqruz
