File:3C58 xray.jpg

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3C58_xray.jpg(576 × 398 pixels, file size: 159 KB, MIME type: image/jpeg)

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Description
English: Chandra's image of 3C58, the remains of a supernova, shows a rapidly rotating neutron star embedded in a cloud of high-energy particles. The data revealed that the neutron star, or pulsar, is rotating about 15 times a second, and is slowing down at the rate of about 10 microseconds per year.
Date
Source http://chandra.harvard.edu/photo/2001/0022/index.html
Author NASA/CXC/SAO/S.Murray et al.
Other versions 0022_xray.tif

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Public domain 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/TimeThumbnailDimensionsUserComment
current05:58, 6 June 2009Thumbnail for version as of 05:58, 6 June 2009576 × 398 (159 KB)Aldebaran66 (talk | contribs){{Information |Description={{en|1=Chandra's image of 3C58, the remains of a supernova observed on Earth in 1181 AD, shows a rapidly rotating neutron star embedded in a cloud of high-energy particles. The data revealed that the neutron star, or pulsar, is

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