File:Big Galaxy Collisions Can Stunt Star Formation (noaoann08023a).tiff
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![File:Big Galaxy Collisions Can Stunt Star Formation (noaoann08023a).tiff](https://upload.wikimedia.org/wikipedia/commons/thumb/1/14/Big_Galaxy_Collisions_Can_Stunt_Star_Formation_%28noaoann08023a%29.tiff/lossy-page1-800px-Big_Galaxy_Collisions_Can_Stunt_Star_Formation_%28noaoann08023a%29.tiff.jpg?20231023223310)
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A deep new image of the Virgo cluster has revealed monumental tendrils of ionized hydrogen gas 400,000 light-years long connecting the elliptical galaxy M86 and the disturbed spiral galaxy NGC 4438.
Summary
[edit]DescriptionBig Galaxy Collisions Can Stunt Star Formation (noaoann08023a).tiff |
English: A deep new image of the Virgo cluster has revealed monumental tendrils of ionized hydrogen gas 400,000 light-years long connecting the elliptical galaxy M86 and the disturbed spiral galaxy NGC 4438. |
Date | 7 October 2008 (upload date) |
Source | Big Galaxy Collisions Can Stunt Star Formation |
Author | Tomer Tal and Jeffrey Kenney/Yale University and NOAO/AURA/NSF |
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current | 22:33, 23 October 2023 | ![]() | 851 × 400 (404 KB) | OptimusPrimeBot (talk | contribs) | #Spacemedia - Upload of https://noirlab.edu/public/media/archives/images/original/noaoann08023a.tif via Commons:Spacemedia |
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Image title | A deep new image of the Virgo cluster has revealed monumental tendrils of ionized hydrogen gas 400,000 light-years long connecting the elliptical galaxy M86 and the disturbed spiral galaxy NGC 4438. |
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Width | 851 px |
Height | 400 px |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Number of rows per strip | 102 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop 21.1 (Windows) |
File change date and time | 00:32, 13 June 2020 |
Exif version | 2.31 |
Color space | Uncalibrated |
Structured data
image/tiff
400 pixel
851 pixel
413,724 byte
e2d8ad109851864ee6700e266a63c3b65da863aa
7 October 2008
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