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
ATCA study of Small Magellanic Cloud supernova remnant 1E 0102.2-7219
Hubble Space Telescope Observations of Oxygen-Rich Supernova Remnants in the Magellanic Cloud. I. Narrow-Band Imaging of N132D in the LMC
Hubble Space Telescope Observations of Oxygen-rich Supernova Remnants in the Magellanic Clouds. II. Elemental Abundances in N132D and 1E 0102.2-7219
Hubble Space Telescope Proper Motion Measurements of Supernova Remnant N132D: Center of Expansion and Age
Polycyclic Aromatic Hydrocarbon Processing in the Blast Wave of the Supernova Remnant N132D
X-Ray-Emitting Ejecta of Supernova Remnant N132D
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-08-09T22:55:16Z/1994-08-10T09:01:56Z
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, Blair comma William P., 1995, 'PROBING EXCITATION MECHANISMS AND ABUNDANCES IN YOUNG MAGELLANIC CLOUD SNRS - CYCLE 4 MED:EARLY ACQ FOR 5607', 1.0, European Space Agency, https://doi.org/10.5270/esa-r5f0ks9