File:Size Comparison Between PSR B1509-58 and Crab Nebula.ogv

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Size_Comparison_Between_PSR_B1509-58_and_Crab_Nebula.ogv(file size: 725 KB, MIME type: application/ogg)

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Summary

Description
English: This animation shows how radio jets may be suppressed in the micro- quasar GRS 1915. Material is being pulled from a red companion star into a black hole via a blue, rapidly rotating disk. The animation begins with a jet blowing material away from the black hole. Later, when the disk is heated by powerful radiation from close to the black hole, a wind is driven off the disk. As the wind strengthens, the jet apparently is shut down because the wind deprives the jet of material that would otherwise have fuelled it.
Date
Source CHANDRA Photo Album
Author B1509-58 (NASA/CXC/SAO/P.Slane, et al.); Crab (NASA/CXC/SAO/F.Seward et al.)
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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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2 May 2010

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current02:25, 2 May 2010 (725 KB)imagescommonswiki>Originalwana{{Information |Description={{en|1=This animation shows how radio jets may be suppressed in the micro- quasar GRS 1915. Material is being pulled from a red companion star into a black hole via a blue, rapidly rotating disk. Th

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