Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-dominated Shells
Imagery and UV Spectroscopy of the LMC Supernova Remnant N103B Using HST
Integral Field Spectroscopy of Balmer-dominated Shocks in the Magellanic Cloud Supernova Remnant N103B
Nature of the Diffuse Source and Its Central Point-like Source in SNR 0509-67.5
Physical Structures of the Type Ia Supernova Remnant N103B
Radio emission from interstellar shocks: Young type Ia supernova remnants and the case of N 103B in the Large Magellanic Cloud
Search for Surviving Companions of Progenitors of Young LMC SN Ia Remnants
The impact of satellite trails on Hubble Space Telescope observations
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2013-09-20T17:50:44Z/2014-10-15T18:52:38Z
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, Chu comma You-Hua, 2015, 'A Search for Surviving Companions of Type Ia Supernovae in the Large Magellanic Cloud', 1.0, European Space Agency, https://doi.org/10.5270/esa-jtbkcjd