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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>A short review on the pulsar magnetic inclination angles · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2404.13857/</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/2404.13857/feed.xml" rel="self" type="application/rss+xml" /><item><title>A short review on the pulsar magnetic inclination angles — mentioned by dumah</title><link>https://news.ycombinator.com/item?id=44231286</link><guid isPermaLink="false">urn:hackerpapers:mention:2404.13857:44231286</guid><pubDate>Tue, 10 Jun 2025 00:42:59 GMT</pubDate><description>&lt;p&gt;This is called the pulsar’s magnetic inclination and it’s often quite far from 0, all the way to nearly orthogonal. Yes but this is a dynamic process that produces more correlated stars as the galaxy ages. Astronomers routinely measure such parameters using models to provide confidence bounds for their estimates. https://arxiv.org/pdf/2404.13857&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2404.13857/"&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>
