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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Properties of galaxies reproduced by a hydrodynamic simulation · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1405.1418/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/1405.1418/feed.xml" rel="self" type="application/rss+xml" /><item><title>Properties of galaxies reproduced by a hydrodynamic simulation — mentioned by privong</title><link>https://news.ycombinator.com/item?id=7714370</link><guid isPermaLink="false">urn:hackerpapers:mention:1405.1418:7714370</guid><pubDate>Thu, 08 May 2014 08:14:08 GMT</pubDate><description>&lt;p&gt;For context, this project just published a paper in Nature on this simulation [0] and a preprint is available [1]. One of the reasons this simulation is big news is its use of a new numerical technique (a &amp;quot;moving mesh&amp;quot;[2]) for the hydrodynamics which purportedly handles fluid instabilities with much greater accuracy. One effect of this is that cold gas flowing onto galaxies interacts with the hot gas halo around galaxies, which prevents that cold gas from going directly to the centers of galaxies. This results in larger simulated galaxies, which match better with observations. [0]…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1405.1418/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item><item><title>Properties of galaxies reproduced by a hydrodynamic simulation — HN submission</title><link>https://news.ycombinator.com/item?id=7713786</link><guid isPermaLink="false">urn:hackerpapers:submission:1405.1418:7713786</guid><pubDate>Thu, 08 May 2014 03:23:58 GMT</pubDate><description>&lt;p&gt;Properties of galaxies reproduced by a hydrodynamic simulation&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p&gt;2 points; 0 discussion replies on HN. &lt;a href="https://hackerpaper.kaipfister.de/p/1405.1418/"&gt;Paper and source history&lt;/a&gt;. A submission is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item><item><title>Properties of galaxies reproduced by a hydrodynamic simulation — mentioned by privong</title><link>https://news.ycombinator.com/item?id=7713785</link><guid isPermaLink="false">urn:hackerpapers:mention:1405.1418:7713785</guid><pubDate>Thu, 08 May 2014 03:23:41 GMT</pubDate><description>&lt;p&gt;Preprint is now available: http://arxiv.org/abs/1405.1418&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1405.1418/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item></channel></rss>
