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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Spectroscopic evidence for a large spot on the dimming Betelgeuse · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2108.03472/</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/2108.03472/feed.xml" rel="self" type="application/rss+xml" /><item><title>Spectroscopic evidence for a large spot on the dimming Betelgeuse — mentioned by belter</title><link>https://news.ycombinator.com/item?id=36083731</link><guid isPermaLink="false">urn:hackerpapers:mention:2108.03472:36083731</guid><pubDate>Fri, 26 May 2023 13:21:31 GMT</pubDate><description>&lt;p&gt;From this paper : &amp;quot;Spectroscopic evidence for a large spot on the dimming Betelgeuse&amp;quot; - https://arxiv.org/pdf/2108.03472.pdf &amp;quot;Evidence for a large cool spot: What could lead to a temperature drop by 170 K? It should be noted that the lowest temperature obtained on 31-01-2020, Teff = 3476 K, would be one of the coolest effective temperatures measured for a Galactic RSG... According to the stellar evolution theory, the Hayashi limit (the lower limit of Teff for stars in hydrostatic equilibrium) for a star like Betelgeuse is ∼3500 K (see, e.g., Figure 6.5 in 16). Nevertheless, the significance…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2108.03472/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.SR</category></item></channel></rss>
