<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Stars: Imaging | Abel Rosales Page</title><link>https://abelrg25.github.io/es/tags/stars-imaging/</link><atom:link href="https://abelrg25.github.io/es/tags/stars-imaging/index.xml" rel="self" type="application/rss+xml"/><description>Stars: Imaging</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>Stars: Imaging</title><link>https://abelrg25.github.io/es/tags/stars-imaging/</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>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>