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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Observational Cosmology With Semi-Relativistic Stars · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1411.5030/</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/1411.5030/feed.xml" rel="self" type="application/rss+xml" /><item><title>Observational Cosmology With Semi-Relativistic Stars — mentioned by tectonic</title><link>https://news.ycombinator.com/item?id=27020196</link><guid isPermaLink="false">urn:hackerpapers:mention:1411.5030:27020196</guid><pubDate>Sun, 02 May 2021 23:55:53 GMT</pubDate><description>&lt;p&gt;We wrote about this in Orbital Index recently (https://orbitalindex.com) and so I did some background research: Loeb&amp;#x27;s paper [1], mentioned in the article, found that hypervelocity stars accelerated by massive black hole binaries could hypothetically reach as much as *half the speed of light*. This is not something you want to be anywhere near. Relatedly, Chinese astronomers recently published research on 591 high-velocity stars in our galaxy [2, 3], and 43 of these were hypervelocity stars, moving at relativistic speeds and destined to eventually escape the Milky Way entirely. They used…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1411.5030/"&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>
