ATCA study of Small Magellanic Cloud supernova remnant 1E 0102.2-7219
Chandra X-Ray Observatory Arcsecond Imaging of the Young, Oxygen-rich Supernova Remnant 1E 0102.2-7219
Hubble Space Telescope Observations of Oxygen-rich Supernova Remnants in the Magellanic Clouds. II. Elemental Abundances in N132D and 1E 0102.2-7219
Optical Structure and Proper-Motion Age of the Oxygen-rich Supernova Remnant 1E 0102-7219 in the Small Magellanic Cloud
Searching for Surviving Companion in the Young SMC Supernova Remnant 1E 0102.2-7219
Spitzer Observations of the Young Core-Collapse Supernova Remnant 1E0102-72.3: Infrared Ejecta Emission and Dust Formation
The Cas A-like SNR 1E 0102.2-7219 in the Small Magellanic Cloud: An Asymmetric Bipolar Explosion
The Center of Expansion and Age of the Oxygen-rich Supernova Remnant 1E 0102.2-7219
The Expansion of the Forward Shock of 1E 0102.2-7219 in X-Rays
Instrument
FOS/BL, FOS/RD, WFPC2, WFPC2/PC
Temporal Coverage
1995-07-04T04:49:17Z/1996-09-27T03:00:57Z
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, Morse et al., 1997, 'EXCITATION MECHANISMS AND ABUNDANCES IN THE O-RICH SNR E0102.2--7219 IN THE SMC', 1.0, European Space Agency, https://doi.org/10.5270/esa-vk8o9tw