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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Baryons in the Warm-Hot Intergalactic Medium · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/astro-ph_0007217/</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/astro-ph_0007217/feed.xml" rel="self" type="application/rss+xml" /><item><title>Baryons in the Warm-Hot Intergalactic Medium — mentioned by mosesbp</title><link>https://news.ycombinator.com/item?id=44338888</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0007217:44338888</guid><pubDate>Sat, 21 Jun 2025 16:42:29 GMT</pubDate><description>&lt;p&gt;Here is the preprint [1]. From a quick glance, the authors look only at a small (relative to the overall size of the universe) region of space and study the emission from the gas between galaxies (specifically, the WHIM [2]). It would seem challenging to draw major conclusions based on this study - and the authors themselves conclude higher quality data of the type they are using is needed. Some context: This missing gas or &amp;quot;missing baryons&amp;quot; problem is a very old one [3]. See here [4] for a nice review (Section 4 mentions the missing baryons problem, which really is localized to the…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0007217/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph</category></item></channel></rss>
