File:Chandra cometpulsar zoom.jpg
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Chandra_cometpulsar_zoom.jpg (300 × 220 pixels, file size: 13 KB, MIME type: image/jpeg)
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Summary[edit]
| Description |
English: The Chandra image shown (an enlargement of the "Chandra Close-up") reveals a comet-shaped X-ray source well outside the boundary of the supernova remnant. This source consists of a point-like object with a long tail trailing behind it for about 3 light years. ... The point-like X-ray source was discovered by the International Gamma-Ray Astrophysics Laboratory, or INTEGRAL, and is called IGR J11014-6103 (or IGR J11014 for short). ... The elongated emission is pointing towards the center of MSH 11-61A where the pulsar would have been formed. |
| Date | |
| Source | Chandra X-ray Observatory website, url=http://chandra.harvard.edu/photo/2012/igrj11014/. |
| Author | X-ray: NASA/CXC/UC Berkeley/J.Tomsick et al & ESA/XMM-Newton. |
In the Chandra image, seen with XMM-Newton is the faint X-ray tail extending to the top-right. Similar tails have been seen from other pulsars that also do not line up with the pulsar's direction of motion.
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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/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 00:36, 11 March 2013 | | 300 × 220 (13 KB) | Marshallsumter (talk | contribs) | User created page with UploadWizard |
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