<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Cas on 庭 — a journal</title><link>https://www.nichi-doku.de/en/tags/cas/</link><description>Recent content in Cas on 庭 — a journal</description><generator>Hugo</generator><language>en-US</language><lastBuildDate>Sat, 26 Sep 2026 00:00:00 +0000</lastBuildDate><atom:link href="https://www.nichi-doku.de/en/tags/cas/index.xml" rel="self" type="application/rss+xml"/><item><title>Abell 85 — the Garlic Nebula</title><link>https://www.nichi-doku.de/en/astrofotografie/abell-85/</link><pubDate>Sat, 26 Sep 2026 00:00:00 +0000</pubDate><guid>https://www.nichi-doku.de/en/astrofotografie/abell-85/</guid><description>&lt;p&gt;Abell 85, also known as CTB 1, is a large supernova remnant (SNR) located in the constellation Cassiopeia. The southern portion of the remnant&amp;rsquo;s bubble also made it into the Lynds Bright Nebula catalog as LBN 576. Originally catalogued by George Abell as a planetary nebula, it soon became evident that it was in fact an SNR.&lt;/p&gt;&#10;&lt;p&gt;In 2017, the citizen science project Einstein@Home — which normally analyzes gravitational-wave data from the LIGO detector — identified a pulsar within Abell 85: PSR J0002+6216, now known as the &amp;ldquo;Cannonball Pulsar.&amp;rdquo; Travelling at over 1,100 km/s, it&amp;rsquo;s one of the fastest-moving pulsars known — fast enough to eventually leave the Milky Way entirely — and it trails a radio tail roughly 13 light-years long behind it.&lt;/p&gt;</description></item></channel></rss>