<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Metallicity-Luminosity Relation in AGNs |</title><link>https://mrkrmh.github.io/tags/metallicity-luminosity-relation-in-agns/</link><atom:link href="https://mrkrmh.github.io/tags/metallicity-luminosity-relation-in-agns/index.xml" rel="self" type="application/rss+xml"/><description>Metallicity-Luminosity Relation in AGNs</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Fri, 20 Jan 2023 00:00:00 +0000</lastBuildDate><image><url>https://mrkrmh.github.io/media/icon_hu_da05098ef60dc2e7.png</url><title>Metallicity-Luminosity Relation in AGNs</title><link>https://mrkrmh.github.io/tags/metallicity-luminosity-relation-in-agns/</link></image><item><title>Oxygen Abundances &amp; The Metallicity-Luminosity Relation</title><link>https://mrkrmh.github.io/projects/oxygen-abundances/</link><pubDate>Fri, 20 Jan 2023 00:00:00 +0000</pubDate><guid>https://mrkrmh.github.io/projects/oxygen-abundances/</guid><description>&lt;p&gt;By systematically analyzing the narrow line regions (NLRs) of Seyfert galaxies, this project explores how actively accreting supermassive black holes influence the gas-phase oxygen abundances in their host environments. Using state-of-the-art photoionization models, we established refined metallicity-luminosity relations crucial for understanding galaxy evolution, specifically noting the anti-correlation driven by AGN feedback.&lt;/p&gt;
&lt;h3 id="interactive-m-z-l-relation-simulator"&gt;Interactive M-Z-L Relation Simulator&lt;/h3&gt;
&lt;p&gt;&lt;em&gt;Simulate the shifts in the Luminosity-Metallicity anti-correlation across varying degrees of AGN feedback strength.&lt;/em&gt;&lt;/p&gt;
&lt;iframe src="https://mrkrmh.github.io/simulations/MZL_Simulator.html" width="100%" height="550px" style="border:none; border-radius: 12px;"&gt;&lt;/iframe&gt;</description></item></channel></rss>