File:Aссretion Spins Pulsar to Millisecond Range.jpg

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English: About 20 km. around, the density of a neutron star attracts matter from a companion star. Inward flowing material causes x-ray bursts and also causes the star's rotation to speed up.
Turkish: Yaklaşık 20 km. çapındaki bir nötron yıldızı yoğunluğundan kaynaklanan kütleçekimiyle eş yıldızındaki maddeyi kendine çekiyor. Eşten pulsara akan gazlar x-ışını patlamalarına neden oluyor. - canlandırma
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Source http://www.nasa.gov/centers/goddard/news/topstory/2003/0702pulsarspeed.html, http://svs.gsfc.nasa.gov/vis/a010000/a010100/a010144/index.html
Author Dana Berry/NASA Goddard Space Flight Center
Other versions File:Millisecond pulsar and accretion disk - NASA animation (hi-res).ogv
File:Millisecond pulsar and accretion disk - NASA animation (low res).ogv
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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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current11:26, 7 September 2013Thumbnail for version as of 11:26, 7 September 20132,880 × 1,944 (1.29 MB)Stas1995 (talk | contribs)User created page with UploadWizard

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