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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>4XMM J181330.1-175110: a new supergiant fast X-ray transient · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2503.04009/</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/2503.04009/feed.xml" rel="self" type="application/rss+xml" /><item><title>4XMM J181330.1-175110: a new supergiant fast X-ray transient — mentioned by wglb</title><link>https://news.ycombinator.com/item?id=43391257</link><guid isPermaLink="false">urn:hackerpapers:mention:2503.04009:43391257</guid><pubDate>Mon, 17 Mar 2025 18:18:10 GMT</pubDate><description>&lt;p&gt;&amp;quot;Italian astronomers report the detection of a new X-ray binary (XRB), which has received the designation 4XMM J181330.1-17511 (J1813 for short). The newfound object represents the rare subclass of XRBs known as supergiant fast X-ray transients. The discovery is detailed in a research paper published March 6 on the arXiv preprint server.&amp;quot; The paper is at https://arxiv.org/abs/2503.04009. I&amp;#x27;ve been long fascinated by odd astronomical items like this, particularly since I heard Joe Taylor play an audio tape of various frequencies that quasars pulsed at.&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2503.04009/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item></channel></rss>
