File:G327.1-1.1.png
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| Description |
English: The Chandra image of the supernova remnant G327.1-1.1 shows the outward-moving, or forward, shock wave (seen as the faint red color), and a bright pulsar wind nebula (blue). The pulsar wind nebula appears to have been distorted by the combined action of the reverse shock wave, which may have flattened it, and by the motion of the pulsar, which created a comet, or lobster-like tail. |
| Date | |
| Source | https://chandra.harvard.edu/photo/2014/msh11g327/ |
| Author | Chandra X-ray Observatory |
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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 | |
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| current | 10:32, 6 October 2021 | | 605 × 603 (442 KB) | Fran Ara (talk | contribs) | Uploaded a work by Chandra X-ray Observatory from https://chandra.harvard.edu/photo/2014/msh11g327/ with UploadWizard |
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