<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Galaxies: Stellar Content | Borja Perez-Diaz</title><link>https://borja-perez-diaz.github.io/me/tags/galaxies-stellar-content/</link><atom:link href="https://borja-perez-diaz.github.io/me/tags/galaxies-stellar-content/index.xml" rel="self" type="application/rss+xml"/><description>Galaxies: Stellar Content</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Mon, 01 Apr 2024 00:00:00 +0000</lastBuildDate><image><url>https://borja-perez-diaz.github.io/me/media/icon_hu7729264130191091259.png</url><title>Galaxies: Stellar Content</title><link>https://borja-perez-diaz.github.io/me/tags/galaxies-stellar-content/</link></image><item><title>Exploring the hardness of the ionising radiation with the infrared softness diagram. I. Similar effective temperature scales for starbursts and (ultra)luminous infrared galaxies</title><link>https://borja-perez-diaz.github.io/me/publication/2024-aa-684-a-40-p/</link><pubDate>Mon, 01 Apr 2024 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2024-aa-684-a-40-p/</guid><description/></item><item><title>The softness diagram for MaNGA star-forming regions: diffuse ionized gas contamination or local HOLMES predominance?</title><link>https://borja-perez-diaz.github.io/me/publication/2023-aa-669-a-88-p/</link><pubDate>Sun, 01 Jan 2023 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2023-aa-669-a-88-p/</guid><description/></item></channel></rss>