A Comparison of X-Ray and Optical Emission in Cassiopeia A
A hyperspectral view of Cassiopeia A
Discovery of Outlying High-Velocity Oxygen-Rich Ejecta in Cassiopeia A
Ejecta Knot Flickering, Mass Ablation, and Fragmentation in Cassiopeia A
Hubble Space Telescope WFPC2 Imaging of Cassiopeia A
Location of the Optical Reverse Shock in the Cassiopeia A Supernova Remnant
Search for a Near-Infrared Counterpart to the Cassiopeia A X-Ray Point Source
Spitzer IRAC Images and Sample Spectra of Cassiopeia As Explosion
The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant
The Identification of Infrared Synchrotron Radiation from Cassiopeia A
The Polar Regions of Cassiopeia A: The Aftermath of a Gamma-Ray Burst?
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2000-01-22T12:40:14Z/2000-01-23T20:39:34Z
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 et al., 2001, 'The Spatial and Ionization Structure of Cas A's Metal-Rich Ejecta', 1.0, European Space Agency, https://doi.org/10.5270/esa-0fvr0gr