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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>NS 1987A in SN 1987A · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2004.06078/</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/2004.06078/feed.xml" rel="self" type="application/rss+xml" /><item><title>NS 1987A in SN 1987A — mentioned by sradman</title><link>https://news.ycombinator.com/item?id=24092135</link><guid isPermaLink="false">urn:hackerpapers:mention:2004.06078:24092135</guid><pubDate>Sat, 08 Aug 2020 15:05:08 GMT</pubDate><description>&lt;p&gt;The paper NS 1987A in SN 1987A [1] claims that Super Nova SN 1987A most likely created a Neutron Star (NS 1987A): &amp;gt; The suspected detection stems from an excess of infrared emission from a dust blob near the compact object’s predicted position. [1] https://arxiv.org/pdf/2004.06078.pdf&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2004.06078/"&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>
