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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9 · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1702.02167/</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/1702.02167/feed.xml" rel="self" type="application/rss+xml" /><item><title>The ultracompact nature of the black hole candidate X-ray binary 47 Tuc X9 — mentioned by jpmattia</title><link>https://news.ycombinator.com/item?id=13886018</link><guid isPermaLink="false">urn:hackerpapers:mention:1702.02167:13886018</guid><pubDate>Thu, 16 Mar 2017 15:51:04 GMT</pubDate><description>&lt;p&gt;You got me curious, and I wanted to put numbers around this. It&amp;#x27;s worth noting that the actual paper claims only this is a black hole candidate, and is not certain it&amp;#x27;s a black hole (despite the Science alert headline). The paper guesses that the black hole is ~ 1 solar mass, so the Schwarzschild radius would be about 3 km. The distance is about 2.5x the earth-moon, which is about 10^6 km. btw, paper here: https://arxiv.org/pdf/1702.02167.pdf&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1702.02167/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item></channel></rss>
