File:N 63A- Chandra and Hubble - Heic0507f.tif
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Summary
Chandra has imaged the glowing shell created by the destruction of a massive star. X-rays from Chandra (blue), combined with optical (green) and radio (red) data, reveal new details in the supernova remnant, LMC N 63A. The X-ray glow is from material heated to about ten million degrees Celsius by a shock wave generated by the supernova explosion. The age of the remnant is estimated to be in the range of 2,000 to 5,000 years.
Credit: X-ray: NASA/CXC/Rutgers/J.Warren et al.; Optical: NASA/STScI/U. Ill/Y.Chu; Radio: ATCA/U. Ill/J.Dickel et al.
Colours & filters Band Wavelength Telescope X-ray Chandra Optical Hubble Space Telescope Radio Other
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 12:08, 9 January 2017 | 2,400 × 2,400 (16.5 MB) | 127.0.0.1 (talk) | <p>Chandra has imaged the glowing shell created by the destruction of a massive star. X-rays from Chandra (blue), combined with optical (green) and radio (red) data, reveal new details in the supernova remnant, LMC N 63A. The X-ray glow is from material heated to about ten million degrees Celsius by a shock wave generated by the supernova explosion. The age of the remnant is estimated to be in the range of 2,000 to 5,000 years. </p> <p>Credit: X-ray: NASA/CXC/Rutgers/J.Warren et al.; Optical: NASA/STScI/U. Ill/Y.Chu; Radio: ATCA/U. Ill/J.Dickel et al. </p> <pre>Colours & filters Band Wavelength Telescope X-ray Chandra Optical Hubble Space Telescope Radio Other </pre> <p>. </p> |
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