ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
Hubble Space Telescope Proper Motion Measurements of Supernova Remnant N132D: Center of Expansion and Age
Identification of the central compact object in the young supernova remnant 1E 0102.2-7219
Measuring Dust Production in the Small Magellanic Cloud Core-Collapse Supernova Remnant 1E 0102.2-7219
Optical Structure and Proper-Motion Age of the Oxygen-rich Supernova Remnant 1E 0102-7219 in the Small Magellanic Cloud
Polycyclic Aromatic Hydrocarbon Processing in the Blast Wave of the Supernova Remnant N132D
Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-7219
Spitzer Space Telescope observations of dust in the Small Magellanic Cloud
The Center of Expansion and Age of the Oxygen-rich Supernova Remnant 1E 0102.2-7219
The impact of satellite trails on Hubble Space Telescope observations
Three-dimensional Kinematic Reconstruction of the Optically Emitting, High-velocity, Oxygen-rich Ejecta of Supernova Remnant N132D
X-Ray-Emitting Ejecta of Supernova Remnant N132D
Instrument
ACS, ACS/WFC
Temporal Coverage
2003-10-15T19:52:52Z/2004-01-22T02:44:49Z
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, Green et al., 2005, 'Emission-line Imaging of Young SNRs in the Magellanic Clouds', 1.0, European Space Agency, https://doi.org/10.5270/esa-a3acrz9
