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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Mapping Milky Way disk perturbations in stellar number density and vertical velocity using Gaia DR3 · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2207.03492/</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/2207.03492/feed.xml" rel="self" type="application/rss+xml" /><item><title>Mapping Milky Way disk perturbations in stellar number density and vertical velocity using Gaia DR3 — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=32686353</link><guid isPermaLink="false">urn:hackerpapers:mention:2207.03492:32686353</guid><pubDate>Fri, 02 Sep 2022 03:45:43 GMT</pubDate><description>&lt;p&gt;You probably can&amp;#x27;t, because your parent comment&amp;#x27;s figure is too large and too precise. You can get some maps at e.g. &amp;lt;https://en.wikipedia.org/wiki/List_of_nearest_stars_and_brow...&amp;gt; and more if you explore through the cited papers. There are 10 known stars or star-systems within approximately 10 light-years of our local star (Proxima Centauri, the Alpha Centauri triple, Barnard&amp;#x27;s star, Luhman 16 in Vela, W0855 in Hydra, Wolf 359 in Leo, Gilese 411 in Ursa Major, the Sirius binary, and the UL Ceti / BV Ceti binary and right on the edge of our 10 light-year bubble V1216 Sagittari). There are…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2207.03492/"&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>
