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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>A Swift survey of accretion onto stellar-mass black holes · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1112.2249/</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/1112.2249/feed.xml" rel="self" type="application/rss+xml" /><item><title>A Swift survey of accretion onto stellar-mass black holes — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=15715691</link><guid isPermaLink="false">urn:hackerpapers:mention:1112.2249:15715691</guid><pubDate>Thu, 16 Nov 2017 19:26:28 GMT</pubDate><description>&lt;p&gt;&amp;gt; AFAIK, only supermassive black holes at the center of galaxies have disks of material that is falling inward Stellar binaries are extremely common, and there is a reasonably large supply of binarys where one star has become a compact object. Their companion stars often drop lots of matter onto them, resulting in a reasonable supply of black holes. Diskoseismologists and others working on Swift have catalogued hundreds of stellar mass black hole accretion disks. Examples from Swift: http://adsabs.harvard.edu/abs/2013ApJ...769...16R https://arxiv.org/abs/1112.2249 (preprint version) Swift…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1112.2249/"&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>
