File:Chandra cometpulsar zoomFairUse.jpg
Chandra_cometpulsar_zoomFairUse.jpg (300 × 220 pixels, file size: 13 KB, MIME type: image/jpeg)
Summary edit
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.
Licensing edit
Description |
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. |
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Source |
The image appears on a website entitled, "Chandra Photo Album IGR J11014-6103" at url=http://chandra.harvard.edu/photo/2012/igrj11014/. |
Date |
28 June 2012 |
Author |
X-ray: NASA/CXC/UC Berkeley/J.Tomsick et al & ESA/XMM-Newton |
Permission (Reusing this file) |
See below |
This file is in the public domain because it was created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (NASA copyright policy page or JPL Image Use Policy). |
Warnings:
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 16:40, 4 July 2015 | 300 × 220 (13 KB) | Marshallsumter (discuss | contribs) | 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... |
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