File:How Black Hole Winds Blow (Artist's Concept).jpg

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English: Supermassive black holes at the cores of galaxies blast radiation and ultra-fast winds outward, as illustrated in this artist's conception. New data from NASA's Nuclear Spectroscopic Telescope Array (NuSTAR) and the European Space Agency's (ESA's) XMM-Newton telescopes show that these winds, which contain gases of highly ionized atoms, blow in a nearly spherical fashion, emanating in every direction, as shown in the artwork. The findings rule out the possibility that the winds blow in narrow beams. With the shape and extent of the winds known, the researchers were able to determine the winds' strength. The high-speed winds are powerful enough to shut down star formation throughout a galaxy.
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Source https://photojournal.jpl.nasa.gov/catalog/PIA18919
Author NASA/JPL-Caltech

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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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current19:28, 9 September 2023Thumbnail for version as of 19:28, 9 September 20234,267 × 2,400 (1.57 MB)Юрий Д.К. (talk | contribs)Uploaded a work by NASA/JPL-Caltech from https://photojournal.jpl.nasa.gov/catalog/PIA18919 with UploadWizard

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