A Direct Measurement of the Forward Shock Speed in Supernova Remnant 0509-67.5: Constraints on the Age, Ambient Density, Shock Compression Factor, and Electron-ion Temperature Equilibration
A Hydro-based MCMC Analysis of SNR 0509-67.5: Revealing the Explosion Properties from Fluid Discontinuities Alone
An absence of ex-companion stars in the type Ia supernova remnant SNR 0509-67.5
Constraints on Cosmic-ray Acceleration Efficiency in Balmer Shocks of Two Young Type Ia Supernova Remnants in the Large Magellanic Cloud
Cosmic-ray Acceleration Efficiency versus Temperature Equilibration: The Case of SNR 0509-67.5
Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-dominated Shells
Investigation of the Progenitors of the Type Ia Supernovae Associated with the LMC Supernova Remnants 0505-67.9 and 0509-68.7
Nature of the Diffuse Source and Its Central Point-like Source in SNR 0509-67.5
Radio-continuum study of Large Magellanic Cloud supernova remnant J0509-6731
The Absence of Ex-companions in Type Ia Supernova Remnants
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC, WFPC2, WFPC2/PC
Temporal Coverage
2006-10-28T10:49:44Z/2007-11-07T08:06:37Z
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, Hughes comma John P., 2008, 'The Proper Motion of Supernova Remnant E0509-67.5', 1.0, European Space Agency, https://doi.org/10.5270/esa-9e78i4v
