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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Lifetime and Powers of FR IIs in Galaxy Clusters · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1204.3896/</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/1204.3896/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Lifetime and Powers of FR IIs in Galaxy Clusters — mentioned by antognini</title><link>https://news.ycombinator.com/item?id=41596821</link><guid isPermaLink="false">urn:hackerpapers:mention:1204.3896:41596821</guid><pubDate>Thu, 19 Sep 2024 22:00:43 GMT</pubDate><description>&lt;p&gt;I studied these objects for my first research paper in grad school. (You can see a few images of some of the objects I found in Figure 3 of my paper [1]) In essence the jet blows a hot bubble into the gas that comprises the intracluster medium of the galaxy cluster. Over time synchrotron radiation causes the bubble to cool down and eventually (maybe on the order of a few 100 million to a billion years if I recall right) the bubble comes into thermal equilibrium with the surrounding gas. [1]: https://arxiv.org/pdf/1204.3896&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1204.3896/"&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>
