File:Instabilities in Very Young Neutron Stars- Electron Fraction (SVS48).jpg

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Instabilities_in_Very_Young_Neutron_Stars-_Electron_Fraction_(SVS48).jpg ‎(720 × 528 pixels, file size: 85 KB, MIME type: image/jpeg)

Captions

Captions

Video slate image reads "The following sequence shows the mixing of composition which results from the convective motions. The variable plotted is the electron fraction Ye, which ranges from 0.2 and 0.5."

Summary

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Description
English: Video slate image reads "The following sequence shows the mixing of composition which results from the convective motions. The variable plotted is the electron fraction Ye, which ranges from 0.2 and 0.5."
Date 12 February 1994 (upload date)
Source Instabilities in Very Young Neutron Stars: Electron Fraction
Author NASA's Scientific Visualization Studio - Bruce Fryxell, Pamela ONeil, Adam Burrows
Other versions
  • WEBM version
Keywords
InfoField
Neutron Star; Space science; Supernova; Astrophysics; Density

Licensing

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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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