File:NGC 4636 Background Subtracted (2001-0144-more-1).tiff
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Size of this JPG preview of this TIF file: 800 × 589 pixels. Other resolutions: 320 × 236 pixels | 640 × 471 pixels | 1,024 × 754 pixels | 1,280 × 942 pixels | 1,800 × 1,325 pixels.
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[edit]DescriptionNGC 4636 Background Subtracted (2001-0144-more-1).tiff |
English: NGC 4636 Background Subtracted |
Date | 19 December 2001 (upload date) |
Source | NGC 4636 Background Subtracted |
Author | (Credit: NASA/SAO/CXC/C.Jones et al.) |
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This media is a product of the Chandra X-ray Observatory Credit and attribution belongs to the mission team, if not already specified in the "author" row |
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[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 | 23:04, 16 November 2024 | 1,800 × 1,325 (2.09 MB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://chandra.si.edu/photo/2001/0144/0144_xray_bgsub.tif via Commons:Spacemedia |
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File usage on Commons
The following 5 pages use this file:
- File:NGC 4636- Hot Galactic Arms Point To Vicious Cycle (2001-0144).mpeg
- File:NGC 4636- Hot Galactic Arms Point To Vicious Cycle (2001-0144).pdf
- File:NGC 4636- Hot Galactic Arms Point To Vicious Cycle (2001-0144 - 0144 xray).jpg
- File:NGC 4636- Hot Galactic Arms Point To Vicious Cycle (2001-0144 - 0144 xray).tiff
- File:NGC 4636 Background Subtracted (2001-0144-more-1).jpg
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Image title | This Chandra image of NGC 4636 shows symmetric arms, or arcs, of 10 million degree gas extending 25,000 light years into a cloud of hot gas that surrounds the galaxy. The length and shape of the arms, along with their temperature which is hotter than the surrounding gas cloud, suggest that they are the leading edge of a galaxy-sized shock wave that is racing outward from the center of the galaxy at 700 kilometers per second. The initial outburst is thought to have been triggered by gas falling into a central massive black hole. |
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Author | Chandra X-ray Observatory Center |
Copyright holder | http://chandra.harvard.edu/photo/image_use.html |
Width | 1,800 px |
Height | 1,325 px |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 1 |
Horizontal resolution | 300 dpi |
Vertical resolution | 300 dpi |
Data arrangement | chunky format |
Exif version | 2.21 |
Color space | sRGB |
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image/tiff
1,325 pixel
1,800 pixel
2,193,002 byte
72810f630a53f58b7c529db0aac5c678a738e70c
19 December 2001
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