<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Article-Journal | Abel Rosales Page</title><link>https://abelrg25.github.io/es/publication_types/article-journal/</link><atom:link href="https://abelrg25.github.io/es/publication_types/article-journal/index.xml" rel="self" type="application/rss+xml"/><description>Article-Journal</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>es</language><lastBuildDate>Thu, 01 Aug 2024 00:00:00 +0000</lastBuildDate><image><url>https://abelrg25.github.io/media/icon_hu3560402997257095965.png</url><title>Article-Journal</title><link>https://abelrg25.github.io/es/publication_types/article-journal/</link></image><item><title>A new dimension in the variability of AGB stars: Convection patterns size changes with pulsation</title><link>https://abelrg25.github.io/es/publication/2024-aa-688-a-124-r/</link><pubDate>Thu, 01 Aug 2024 00:00:00 +0000</pubDate><guid>https://abelrg25.github.io/es/publication/2024-aa-688-a-124-r/</guid><description/></item><item><title>An impressionist view of V Hydrae. When MATISSE paints asymmetric giant blobs</title><link>https://abelrg25.github.io/es/publication/2024-aa-687-a-306-p/</link><pubDate>Mon, 01 Jul 2024 00:00:00 +0000</pubDate><guid>https://abelrg25.github.io/es/publication/2024-aa-687-a-306-p/</guid><description/></item><item><title>The dusty circumstellar environment of Betelgeuse during the Great Dimming as seen by VLTI/MATISSE</title><link>https://abelrg25.github.io/es/publication/2023-aa-675-a-46-c/</link><pubDate>Sat, 01 Jul 2023 00:00:00 +0000</pubDate><guid>https://abelrg25.github.io/es/publication/2023-aa-675-a-46-c/</guid><description/></item><item><title>Caracterización de las capas de gas más cercanas a una estrella AGB</title><link>https://abelrg25.github.io/es/publication/journal-article/</link><pubDate>Thu, 01 Jun 2023 00:00:00 +0000</pubDate><guid>https://abelrg25.github.io/es/publication/journal-article/</guid><description>&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-primary-100 dark:bg-primary-900">
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&lt;span class="dark:text-neutral-300">With the advent of high angular resolution techniques, scientists are finding that the innermost environment of AGB stars is asymmetric and changes over short time periods of the order of days.&lt;/span>
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&lt;p>Add the publication&amp;rsquo;s &lt;strong>full text&lt;/strong> or &lt;strong>supplementary notes&lt;/strong> here. You can use rich formatting such as including &lt;a href="https://docs.hugoblox.com/content/writing-markdown-latex/" target="_blank" rel="noopener">code, math, and images&lt;/a>.&lt;/p></description></item><item><title>Imaging the innermost gaseous layers of the Mira star R Car with GRAVITY-VLTI</title><link>https://abelrg25.github.io/es/publication/2023-aa-674-a-62-r/</link><pubDate>Thu, 01 Jun 2023 00:00:00 +0000</pubDate><guid>https://abelrg25.github.io/es/publication/2023-aa-674-a-62-r/</guid><description/></item></channel></rss>