<?xml version="1.0" encoding="UTF-8"?><rss xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:content="http://purl.org/rss/1.0/modules/content/" xmlns:atom="http://www.w3.org/2005/Atom" version="2.0"><channel><title><![CDATA[RSS Feed]]></title><description><![CDATA[RSS Feed]]></description><link>http://direct.ecency.com</link><image><url>http://direct.ecency.com/logo512.png</url><title>RSS Feed</title><link>http://direct.ecency.com</link></image><generator>RSS for Node</generator><lastBuildDate>Thu, 21 May 2026 09:27:44 GMT</lastBuildDate><atom:link href="http://direct.ecency.com/created/estrella-neutrones/rss.xml" rel="self" type="application/rss+xml"/><item><title><![CDATA[J0740 the heaviest known neutron star/J0740 la estrella de neutrones más pesada conocida]]></title><description><![CDATA[Source We have already commented on this blog more than once how stars, when they run out of fuel, go off more or less scandalously from the discrete white dwarf of small stars like the Sun to the black]]></description><link>http://direct.ecency.com/hive-175254/@mauromar/j0740-the-heaviest-known-neutron-star-j0740-la-estrella-de-neutrones-mas-pesada-conocida</link><guid isPermaLink="true">http://direct.ecency.com/hive-175254/@mauromar/j0740-the-heaviest-known-neutron-star-j0740-la-estrella-de-neutrones-mas-pesada-conocida</guid><category><![CDATA[hive-175254]]></category><dc:creator><![CDATA[mauromar]]></dc:creator><pubDate>Tue, 04 May 2021 13:17:03 GMT</pubDate><enclosure url="https://i.ecency.com/p/2N61tyyncFaFrUtdm6XyXa3kXqgNvKhnu9pD2hfz8Qw9b1deEXgJ3AEkve39sqjSp88qdHqMQNgZdgbp58GZFYJNcS7WJYSARL59WFT3DYDGHHvnFuYXtjbiXc5mSY3w57tvPWY878VL?format=match&amp;mode=fit" length="0" type="false"/></item></channel></rss>