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File:N 63A- Chandra and Hubble - Heic0507f.tif

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Description

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
.
Date
Source http://www.spacetelescope.org/images/heic0507f/
Author ESA/Hubble & NASA
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current11:19, 4 May 2012Thumbnail for version as of 11:19, 4 May 20122,400 × 2,400 (16.5 MB)Fabian RRRR{{Information |Description=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-...

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