File:Igrj11014 w22.jpg

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Description
English: X-ray observations from Chandra (green) and XMM-Newton (purple) have been combined such that the large area of diffuse X-rays seen by XMM-Newton was produced when a massive star exploded as a supernova, leaving behind a debris field, or supernova remnant known as SNR MSH 11-16A. Shocks waves from the supernova have heated surrounding gas to several million degrees Kelvin, causing the remnant to glow brightly in X-rays. The point-like X-ray source (Chandra green) was discovered by the International Gamma-Ray Astrophysics Laboratory, or INTEGRAL, and is called IGR J11014-6103 (or IGR J11014 for short).
Date
Source http://chandra.harvard.edu/photo/2012/igrj11014/ (TIFF image link); see also https://xmm-tools.cosmos.esa.int/external/xmm_science/gallery/public/level3.php?id=1153
Author NASA/CXC/UC Berkeley/J.Tomsick et al & ESA/XMM-Newton

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Date/TimeThumbnailDimensionsUserComment
current09:59, 2 July 2017Thumbnail for version as of 09:59, 2 July 20173,600 × 2,894 (396 KB)Huntster (talk | contribs)Full resolution.
00:15, 11 March 2013Thumbnail for version as of 00:15, 11 March 2013525 × 422 (71 KB)Marshallsumter (talk | contribs)User created page with UploadWizard

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