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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Phosphorus Abundances in FGK Stars · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1704.08282/</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/1704.08282/feed.xml" rel="self" type="application/rss+xml" /><item><title>Phosphorus Abundances in FGK Stars — mentioned by bigbillheck</title><link>https://news.ycombinator.com/item?id=38660438</link><guid isPermaLink="false">urn:hackerpapers:mention:1704.08282:38660438</guid><pubDate>Sat, 16 Dec 2023 00:12:23 GMT</pubDate><description>&lt;p&gt;&amp;gt; it is noteworthy to find a star that has it. I don&amp;#x27;t think this is an accurate reading of that article. See forex https://arxiv.org/abs/1704.08282 whose abstract reads in part: &amp;gt; We also found average [P/Si] = 0.02 ± 0.07 and [P/S] = 0.15 ± 0.15 for our sample, showing no significant deviations from the solar ratios for [P/Si] and [P/S] ratios. Quoting from the introduction I find: Phosphorus abundances have been derived in planetary nebulae .... and in damped Lyman alpha systems using ionized phosphorus lines ... Anomalously high phosphorus abundances have been measured using optical…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1704.08282/"&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>
