위키백과 ― 우리 모두의 백과사전.
Description |
This image of spiral galaxy NGC 3627, also known as Messier 66, was captured by the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC).
The SINGS image is a four-channel false-color composite, where blue indicates emission at 3.6 microns, green corresponds to 4.5 microns, and red to 5.8 and 8.0 microns. The contribution from starlight (measured at 3.6 microns) in this picture has been subtracted from the 5.8 and 8 micron images to enhance the visibility of the polycyclic aromatic hydrocarbon emission
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Source |
http://sscws1.ipac.caltech.edu/Imagegallery/image.php?image_name=sig05-016
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Date |
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Author |
NASA
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Other versions |
Originally from en.wikipedia; description page is (was) here
* 03:38, 4 September 2006 [[:en:User:WilliamKF|WilliamKF]] 812×812 (588,791 bytes) <span class="comment">(This image of spiral galaxy NGC 3627, also known as Messier 66, was captured by the Spitzer Infrared Nearby Galaxy Survey (SINGS) Legacy Project using the telescope's Infrared Array Camera (IRAC). The SINGS image is a four-channel false-color composite, )</span> |
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