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Bild:Sig05-005.jpg – Wikipedia

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[edit] Summary

High resolution images from NASA's Spitzer infrared telescope and GALEX ultraviolet telescope show the difference in the distribution of young and old stars in the Arp 65 pair of interacting galaxies. In the short-wavelength infrared at 3.6 microns (first image), cool old stars are bright, so the beautiful grand design spiral patterns in the old stellar disks are visible. In contrast, at longer infrared wavelengths, at 8 microns, bright clumps of young stars are detected (second image). The difference in distribution between the old and young stellar populations is clear in the third image, where the 3.6 micron (blue) and 8.0 micron (red) images are combined. This clumpy structure is also present in the ultraviolet, as revealed in the GALEX ultraviolet images (fourth image, with near-ultraviolet in yellow and far-ultraviolet in blue).

These images were presented at the American Astronomical Society meeting in Minneapolis, Minnesota, on May 30, 2005

[edit] File info

Description

Interacting Galaxy Pair Arp 65

Source

http://gallery.spitzer.caltech.edu/Imagegallery/image.php?image_name=sig05-005

Date

2005/06/09

Author

NASA/JPL-Caltech/M. L. Giroux (East Tennessee State University)

Permission
(Reusing this image)

http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml


[edit] Individual images

see http://gallery.spitzer.caltech.edu/Imagegallery/image.php?image_name=sig05-005 High quality tif files also avaliable.


[edit] Licensing

Public domain
This file is in the public domain because it was created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (NASA copyright policy page or JPL Image Use Policy).

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aktuell00:43, 10. Jul. 20071.500×1.200 (1,37 MB)Anzibanonzi (==Summary== High resolution images from NASA's Spitzer infrared telescope and GALEX ultraviolet telescope show the difference in the distribution of young and old stars in the Arp 65 pair of interacting galaxies. In the short-wavelength infrared at 3.6 mi)

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