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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Black Hole Mass Distribution in the Galaxy · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1006.2834/</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/1006.2834/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Black Hole Mass Distribution in the Galaxy — mentioned by shagie</title><link>https://news.ycombinator.com/item?id=39365388</link><guid isPermaLink="false">urn:hackerpapers:mention:1006.2834:39365388</guid><pubDate>Wed, 14 Feb 2024 01:49:20 GMT</pubDate><description>&lt;p&gt;The next problem is https://arxiv.org/pdf/1006.2834.pdf which has the lightest black holes at 5.0⊙ There&amp;#x27;s another interesting object - https://www.science.org/doi/10.1126/science.adg3005 This is a binary system with a total mass of 3.887⊙ ± 0.004 ... which puts the companion in the system at 2.09⊙ to 2.71⊙ ... which may be in the &amp;quot;heavier than any theoretical neutron star, but lighter than any known black hole. A recent Dr. Becky video on this: FOUND in the MASS GAP: The heaviest neutron star OR the lightest black hole? https://youtu.be/8PHt7NcwllA&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1006.2834/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.GA</category></item></channel></rss>
