<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Infrared: ISM | Borja Perez-Diaz</title><link>https://borja-perez-diaz.github.io/me/tags/infrared-ism/</link><atom:link href="https://borja-perez-diaz.github.io/me/tags/infrared-ism/index.xml" rel="self" type="application/rss+xml"/><description>Infrared: ISM</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 01 May 2024 00:00:00 +0000</lastBuildDate><image><url>https://borja-perez-diaz.github.io/me/media/icon_hu7729264130191091259.png</url><title>Infrared: ISM</title><link>https://borja-perez-diaz.github.io/me/tags/infrared-ism/</link></image><item><title>Chemical abundances and deviations from the solar S/O ratio in the gas-phase interstellar medium of galaxies based on infrared emission lines</title><link>https://borja-perez-diaz.github.io/me/publication/2024-aa-685-a-168-p/</link><pubDate>Wed, 01 May 2024 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2024-aa-685-a-168-p/</guid><description/></item><item><title>Measuring chemical abundances in AGN from infrared nebular lines: HII-CHI-MISTRY-IR for AGN</title><link>https://borja-perez-diaz.github.io/me/publication/2022-aa-666-a-115-p/</link><pubDate>Sat, 01 Oct 2022 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2022-aa-666-a-115-p/</guid><description/></item></channel></rss>