File:Zwicky 8338.jpg
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DescriptionZwicky 8338.jpg |
English: An extraordinary ribbon of hot gas trailing behind a galaxy like a tail has been discovered using data from NASA's Chandra X-ray Observatory. This ribbon, or X-ray tail, is likely due to gas stripped from the galaxy as it moves through a vast cloud of hot intergalactic gas. With a length of at least 250,000 light years, it is likely the largest such tail ever detected. The newly discovered tail is seen in this composite image of X-rays (blue) and optical data (yellow). |
Date | |
Source | http://chandra.si.edu/photo/2015/z8338/ |
Author | NASA/Chandra X-ray Telescope |
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Public domainPublic domainfalsefalse |
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 | 17:19, 29 December 2015 | 864 × 864 (745 KB) | Mylkomeda (talk | contribs) | User created page with UploadWizard |
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Image title |
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Author | Chandra X-ray Observatory Center |
Source | Chandra X-ray Observatory |
Headline | A galaxy cluster located almost 700 million light years from Earth. |
Credit/Provider | X-ray: NASA/CXC/University of Bonn/G. Schellenberger et al; Optical: INT |
Short title |
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Usage terms | |
Date and time of data generation | 21 December 2015 |
Orientation | Normal |
Horizontal resolution | 0.005952380952381 dpi |
Vertical resolution | 0.00031111111111111 dpi |
File change date and time | (Macintosh) |
Exif version | 2.21 |
Color space | sRGB |
Software used | Adobe Photoshop CS6 (Macintosh) |
Rating (out of 5) | 0 |
Date metadata was last modified | 06:33, 21 December 2015 |
Date and time of digitizing | 06:37, 17 November 2015 |
Unique ID of original document | 9DB3FB4E6EE9D28A8AF22525BAD09D37 |
Keywords | Zwicky 8338 |
Contact information | cxcpub@cfa.harvard.edu
60 Garden St. Cambridge, MA, 02138 USA |
IIM version | 4 |