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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1311.2073/</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/1311.2073/feed.xml" rel="self" type="application/rss+xml" /><item><title>Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation — mentioned by privong</title><link>https://news.ycombinator.com/item?id=12461336</link><guid isPermaLink="false">urn:hackerpapers:mention:1311.2073:12461336</guid><pubDate>Fri, 09 Sep 2016 11:58:34 GMT</pubDate><description>&lt;p&gt;&amp;gt; Can somebody who knows about this tell me how much of the novelty in this is CS and how much physics? It&amp;#x27;s a little bit of both. Over the past 5–8 years, some new numerical techniques (&amp;quot;moving mesh&amp;quot;) have been developed (or at least first applied in astronomy) for hydrodynamic simulations[0,1]. These new techniques do a much better job of handling fluid instabilities, which can be important for properly simulating the gas in galaxies (which can have a huge range in densities and temperatures). Also, people have developed what they call &amp;quot;cosmological zoom&amp;quot; simulations. In these simulations…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1311.2073/"&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>Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation — mentioned by privong</title><link>https://news.ycombinator.com/item?id=9163246</link><guid isPermaLink="false">urn:hackerpapers:mention:1311.2073:9163246</guid><pubDate>Sat, 07 Mar 2015 21:50:11 GMT</pubDate><description>&lt;p&gt;I was expecting the actual game, not just a video about it, but it does look interesting. It&amp;#x27;s also worth noting that much of what is included in the game is still actively being researched. For example, we don&amp;#x27;t really know, in detail, how vigorous star formation affects the gas in galaxies – is it expelled, stirred up, removed from the system, or some combination? And what processes (supernovae, stellar winds, radiation pressure, etc.) drive that? I think we are getting close to the answers[0, 1], but it&amp;#x27;s an exciting time. [0] http://arxiv.org/abs/1311.2073 [1]…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1311.2073/"&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>
