<?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, Interferometry, AGB and Post-AGB Stars, Winds, Outflows, Atmospheres | Abel Rosales Page</title><link>https://abelrg25.github.io/es/tags/high-angular-resolution-techniques-interferometry-agb-and-post-agb-stars-winds-outflows-atmospheres/</link><atom:link href="https://abelrg25.github.io/es/tags/high-angular-resolution-techniques-interferometry-agb-and-post-agb-stars-winds-outflows-atmospheres/index.xml" rel="self" type="application/rss+xml"/><description>High Angular Resolution Techniques, Interferometry, AGB and Post-AGB Stars, Winds, Outflows, Atmospheres</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>es</language><lastBuildDate>Thu, 01 Jun 2023 00:00:00 +0000</lastBuildDate><image><url>https://abelrg25.github.io/media/icon_hu3560402997257095965.png</url><title>High Angular Resolution Techniques, Interferometry, AGB and Post-AGB Stars, Winds, Outflows, Atmospheres</title><link>https://abelrg25.github.io/es/tags/high-angular-resolution-techniques-interferometry-agb-and-post-agb-stars-winds-outflows-atmospheres/</link></image><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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