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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The origin of the young stellar population in the solar neighborhood - a link to the formation of the Local Bubble? · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/astro-ph_0205128/</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_0205128/feed.xml" rel="self" type="application/rss+xml" /><item><title>The origin of the young stellar population in the solar neighborhood - a link to the formation of the Local Bubble? — mentioned by antonvs</title><link>https://news.ycombinator.com/item?id=24655984</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0205128:24655984</guid><pubDate>Thu, 01 Oct 2020 20:45:12 GMT</pubDate><description>&lt;p&gt;The Local Bubble is thought to have been caused my multiple supernovae. See e.g. this 2002 paper: https://arxiv.org/abs/astro-ph/0205128v2 Edit: Here&amp;#x27;s a more recent paper - https://link.springer.com/referenceworkentry/10.1007%2F978-3... : &amp;gt; &amp;quot;More detailed models for the origins of the Local Bubble have found that it requires anywhere from 3 (Smith and Cox 2001) to 20 (Fuchs et al. 2006) SNe to create a bubble with the correct characteristics in terms of size, pressure, and emission characteristics.&amp;quot;&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0205128/"&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>
