A Comparison of X-Ray and Optical Emission in Cassiopeia A
A hyperspectral view of Cassiopeia A
Coronal emission from the shocked circumstellar ring of SN 1987A
Discovery of Outlying High-Velocity Oxygen-Rich Ejecta in Cassiopeia A
Ejecta Knot Flickering, Mass Ablation, and Fragmentation in Cassiopeia A
Location of the Optical Reverse Shock in the Cassiopeia A Supernova Remnant
No surviving non-compact stellar companion to Cassiopeia A
The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant
The Polar Regions of Cassiopeia A: The Aftermath of a Gamma-Ray Burst?
The Reverse Shock of SNR 1987A at 18 Years after Outburst
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2002-01-09T00:15:15Z/2002-01-18T22:57:55Z
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, Fesen comma Robert A., 2003, 'The Spatial and Ionization Structure of Cas A's Metal-Rich Ejecta', 1.0, European Space Agency, https://doi.org/10.5270/esa-yfunrfc