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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Licensing

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File history

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Date/TimeThumbnailDimensionsUserComment
current12:08, 9 January 2017Thumbnail for version as of 12:08, 9 January 20172,400 × 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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