A multiwavelength view at the heart of the superwind in NGC253
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Spatially Resolving a Starburst Galaxy at Hard X-Ray Energies: NuSTAR, Chandra, and VLBA Observations of NGC 253
The nucleus of NGC 253 and its massive stellar clusters at parsec scales
The Subparsec-Scale Radio Properties of Southern Starburst Galaxies. I. Supernova Remnants, the Supernova Rate, and the Ionized Medium in the NGC 253 Starburst
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
1997-07-09T18:56:13Z/1997-07-09T22:48:53Z
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, Forbes comma Duncan A., 1998, 'Resolving the Radio Hotspots in Nearby Starburst Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-lfnatkc