<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Galaxies: Abundances | Borja Perez-Diaz</title><link>https://borja-perez-diaz.github.io/me/tags/galaxies-abundances/</link><atom:link href="https://borja-perez-diaz.github.io/me/tags/galaxies-abundances/index.xml" rel="self" type="application/rss+xml"/><description>Galaxies: Abundances</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Sat, 01 Feb 2025 00:00:00 +0000</lastBuildDate><image><url>https://borja-perez-diaz.github.io/me/media/icon_hu7729264130191091259.png</url><title>Galaxies: Abundances</title><link>https://borja-perez-diaz.github.io/me/tags/galaxies-abundances/</link></image><item><title>Chemical enrichment in LINERs from MaNGA: I. Tracing the nuclear abundances of oxygen and nitrogen in LINERs with varied ionizing sources</title><link>https://borja-perez-diaz.github.io/me/publication/2025-aa-694-a-18-p/</link><pubDate>Sat, 01 Feb 2025 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2025-aa-694-a-18-p/</guid><description/></item><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>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>Assessing model-based carbon and oxygen abundance derivation from ultraviolet emission lines in AGNs</title><link>https://borja-perez-diaz.github.io/me/publication/2023-mnras-521-1556-p/</link><pubDate>Mon, 01 May 2023 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2023-mnras-521-1556-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><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><item><title>Chemical abundances in the nuclear region of nearby galaxies from the Palomar Survey</title><link>https://borja-perez-diaz.github.io/me/publication/2021-mnras-505-4289-p/</link><pubDate>Sun, 01 Aug 2021 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/me/publication/2021-mnras-505-4289-p/</guid><description/></item></channel></rss>