<?xml version="1.0"?>
<feed xmlns="http://www.w3.org/2005/Atom" xml:lang="en">
	<id>https://selfgravitatingfluids.education/JETohline/index.php?action=history&amp;feed=atom&amp;title=ThreeDimensionalConfigurations%2FChallenges</id>
	<title>ThreeDimensionalConfigurations/Challenges - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://selfgravitatingfluids.education/JETohline/index.php?action=history&amp;feed=atom&amp;title=ThreeDimensionalConfigurations%2FChallenges"/>
	<link rel="alternate" type="text/html" href="https://selfgravitatingfluids.education/JETohline/index.php?title=ThreeDimensionalConfigurations/Challenges&amp;action=history"/>
	<updated>2026-04-22T09:53:59Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.43.1</generator>
	<entry>
		<id>https://selfgravitatingfluids.education/JETohline/index.php?title=ThreeDimensionalConfigurations/Challenges&amp;diff=1854&amp;oldid=prev</id>
		<title>Joel2: Created page with &quot;__FORCETOC__&lt;!--  will force the creation of a Table of Contents --&gt; &lt;!-- __NOTOC__ will force TOC off --&gt; =Challenges Constructing Ellipsoidal-Like Configurations= First, let&#039;s review the three different approaches that we have described for constructing Riemann S-type ellipsoids.  Then let&#039;s see how these relate to the technique that has been used to construct infinitesimally thin, nonaxisymmetric disks.    ==Riemann S-type Ellipsoids==  Usually, the density, &lt;math&gt;~\r...&quot;</title>
		<link rel="alternate" type="text/html" href="https://selfgravitatingfluids.education/JETohline/index.php?title=ThreeDimensionalConfigurations/Challenges&amp;diff=1854&amp;oldid=prev"/>
		<updated>2024-07-03T22:47:48Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;__FORCETOC__&amp;lt;!--  will force the creation of a Table of Contents --&amp;gt; &amp;lt;!-- __NOTOC__ will force TOC off --&amp;gt; =Challenges Constructing Ellipsoidal-Like Configurations= First, let&amp;#039;s review the three different approaches that we have described for constructing Riemann S-type ellipsoids.  Then let&amp;#039;s see how these relate to the technique that has been used to construct infinitesimally thin, nonaxisymmetric disks.    ==Riemann S-type Ellipsoids==  Usually, the density, &amp;lt;math&amp;gt;~\r...&amp;quot;&lt;/p&gt;
&lt;a href=&quot;https://selfgravitatingfluids.education/JETohline/index.php?title=ThreeDimensionalConfigurations/Challenges&amp;amp;diff=1854&quot;&gt;Show changes&lt;/a&gt;</summary>
		<author><name>Joel2</name></author>
	</entry>
</feed>