A Catalog of Outer Ejecta Knots in the Cassiopeia A Supernova Remnant
A Comparison of X-Ray and Optical Emission in Cassiopeia A
A Detailed Kinematic Map of Cassiopeia As Optical Main Shell and Outer High-velocity Ejecta
An HST Survey of the Highest-velocity Ejecta in Cassiopeia A
Discovery of Outlying High-Velocity Oxygen-Rich Ejecta in Cassiopeia A
Ejecta Knot Flickering, Mass Ablation, and Fragmentation in Cassiopeia A
Fine-structure infrared lines from the Cassiopeia A knots
Near-Infrared Knots and Dense Fe Ejecta in the Cassiopeia A Supernova Remnant
No surviving non-compact stellar companion to Cassiopeia A
The bubble-like interior of the core-collapse supernova remnant Cassiopeia A
The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant
The impact of satellite trails on Hubble Space Telescope observations
The Nature of the Ultraluminous Oxygen-Rich Supernova Remnant in NGC 4449
The Shape of Cas A
Instrument
ACS, ACS/WFC
Temporal Coverage
2004-12-04T12:07:21Z/2004-12-05T16:22:04Z
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., 2005, 'Probing the Dynamics and Shock Physics of the Cas A Supernova Remnant', 1.0, European Space Agency, https://doi.org/10.5270/esa-barmauh