File:ChandrasekharLimitGraph sv.svg

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English: Graph plotting the radius (in standard solar radii) against the mass (in standard solar masses) for a model white dwarf star consisting of a cold Fermi gas. The blue curve shows a nonrelativistic model and the green curve a relativistic model. The molecular weight per electron has been taken to be 2. See: The Highly Collapsed Configurations of a Stellar Mass (second paper), S. Chandrasekhar, Monthly Notices of the Royal Astronomical Society, 95 (1935), pp. 207--225.
Svenska: Plottning av radie (i solradier) och massa (i solmassor) av en vit dvärg bestående av kall Fermigas. Den blå kurvan visar en ickerelativistisk modell medan the gröna kurvan visar den relativistiska modellen. Molekylärvikten per atom antas vara 2.
Date (UTC)
Source ChandrasekharLimitGraph.svg
Author Warrakkk after original by Chrkl


This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: Swedish version. The original can be viewed here: ChandrasekharLimitGraph.svg. Modifications made by Warrakkk.

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  • File:ChandrasekharLimitGraph.svg licensed with PD-self
    • 2010-02-03T12:46:54Z Chrkl 1052x744 (31117 Bytes) {{Information |Description={{mld |de=Englischsprachige Version eines Graphen, der den Radius (in Standard-Sonnenradien) eines beispielhaften, aus kaltem Fermigas bestehenden weißen Zwerges in Relation zur Masse (in Standard

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Date/TimeThumbnailDimensionsUserComment
current11:18, 24 October 2014Thumbnail for version as of 11:18, 24 October 20141,052 × 744 (26 KB)Svjo (talk | contribs)Reverted to version as of 21:28, 10 March 2010
11:13, 24 October 2014Thumbnail for version as of 11:13, 24 October 2014938 × 707 (36 KB)Svjo (talk | contribs)text size
21:28, 10 March 2010Thumbnail for version as of 21:28, 10 March 20101,052 × 744 (26 KB)MickOhrberg (talk | contribs){{Information |Description={{mld |en=Graph plotting the radius (in standard solar radii) against the mass (in standard solar masses) for a model white dwarf star consisting of a cold Fermi gas. The blue curve shows a nonrelativistic model and the green c

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