File:425991main W44 multi.jpg
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[edit]Description425991main W44 multi.jpg |
English: Fermi mapped GeV-gamma-ray emission regions (magenta) in the W44 supernova remnant. The features clearly align with filaments detectable in other wavelengths. This composite merges X-rays (blue) from the Germany-led ROSAT mission, infrared (red) from NASA's Spitzer Space Telescope, and radio (orange) from the Very Large Array near Socorro, N.M. Credit: NASA/DOE/Fermi LAT Collaboration, ROSAT, JPL-Caltech, and NRAO/AUI. |
Date | |
Source | NASA's Fermi Closes on Source of Cosmic Rays, url=http://www.nasa.gov/mission_pages/GLAST/news/cosmic-rays-source.html |
Author | NASA/DOE/Fermi LAT Collaboration, ROSAT, JPL-Caltech, and NRAO/AUI |
Permission (Reusing this file) |
Images from NASA are usually free of copyright and are in the PUBLIC Domain. |
W44 is in the constellation Aquila.
Licensing
[edit]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 | 19:55, 2 May 2011 | 2,119 × 2,400 (4.91 MB) | Marshallsumter (talk | contribs) | {{Information |Description ={{en|1=Fermi mapped GeV-gamma-ray emission regions (magenta) in the W44 supernova remnant. The features clearly align with filaments detectable in other wavelengths. This composite merges X-rays (blue) from the Germany-led R |
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Orientation | Normal |
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Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Software used | Adobe Photoshop CS3 Windows |
File change date and time | 02:20, 11 February 2010 |
Color space | sRGB |
Image width | 2,119 px |
Image height | 2,400 px |
Date and time of digitizing | 21:20, 10 February 2010 |
Date metadata was last modified | 21:20, 10 February 2010 |
IIM version | 7,828 |