<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>High Angular Resolution Techniques, AGB and Post-AGB Stars, Image Reconstruction, R Car | Abel Rosales Page</title><link>https://abelrg25.github.io/es/tags/high-angular-resolution-techniques-agb-and-post-agb-stars-image-reconstruction-r-car/</link><atom:link href="https://abelrg25.github.io/es/tags/high-angular-resolution-techniques-agb-and-post-agb-stars-image-reconstruction-r-car/index.xml" rel="self" type="application/rss+xml"/><description>High Angular Resolution Techniques, AGB and Post-AGB Stars, Image Reconstruction, R Car</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>es</language><lastBuildDate>Mon, 01 Jul 2024 00:00:00 +0000</lastBuildDate><image><url>https://abelrg25.github.io/media/icon_hu3560402997257095965.png</url><title>High Angular Resolution Techniques, AGB and Post-AGB Stars, Image Reconstruction, R Car</title><link>https://abelrg25.github.io/es/tags/high-angular-resolution-techniques-agb-and-post-agb-stars-image-reconstruction-r-car/</link></image><item><title>Convección en estrellas AGB como nunca antes se había visto</title><link>https://abelrg25.github.io/es/publication/conference-paper/</link><pubDate>Mon, 01 Jul 2024 00:00:00 +0000</pubDate><guid>https://abelrg25.github.io/es/publication/conference-paper/</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">If you search for images of the Sun on the internet, you will likely find many showing a granular pattern caused by convective currents. But did you know that evolved stars exhibit gigantic granular patterns? In this article, we show you what these structures look like for an AGB star called R Car&lt;/span>
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