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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Inflation of 430-parsec bipolar radio bubbles in the Galactic Centre by an energetic event · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1909.05534/</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/1909.05534/feed.xml" rel="self" type="application/rss+xml" /><item><title>Inflation of 430-parsec bipolar radio bubbles in the Galactic Centre by an energetic event — mentioned by forgotpwd16</title><link>https://news.ycombinator.com/item?id=21037520</link><guid isPermaLink="false">urn:hackerpapers:mention:1909.05534:21037520</guid><pubDate>Sat, 21 Sep 2019 19:53:33 GMT</pubDate><description>&lt;p&gt;E-print can be found at https://arxiv.org/abs/1909.05534 . Some years ago something similar was found in the form of Fermi bubbles; a discovery given the Bruno Rossi Prize. The difference is the frequencies that the structures were found and their size. Fermi bubbles were identified by γ-ray imagining and are far more massive (many thousands of light years in size); both put together makes them far more energetic as well. An interesting part with this discovery is the correspondence between radio and X-ray emissions in this bipolar radio structure. The radio bubbles appear to exactly bound…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1909.05534/"&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>
