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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The unexpected diversity of dwarf galaxy rotation curves · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1504.01437/</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/1504.01437/feed.xml" rel="self" type="application/rss+xml" /><item><title>The unexpected diversity of dwarf galaxy rotation curves — mentioned by JBorrow</title><link>https://news.ycombinator.com/item?id=18751176</link><guid isPermaLink="false">urn:hackerpapers:mention:1504.01437:18751176</guid><pubDate>Mon, 24 Dec 2018 08:49:10 GMT</pubDate><description>&lt;p&gt;Yeah, in fact we simulate many thousands of galaxies all at once in a big cosmological volume and they all have very realistic rotation curves -- we match these to the observed rotation curves of galaxies, or use them to make predictions about galaxies that we have not yet observed. See e.g. Fig 1. in this paper: https://arxiv.org/pdf/1504.01437.pdf&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1504.01437/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.GA</category></item></channel></rss>
