<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Teaching | Borja Perez-Diaz | Doctor in Astrophysics</title><link>https://borja-perez-diaz.github.io/teaching/</link><atom:link href="https://borja-perez-diaz.github.io/teaching/index.xml" rel="self" type="application/rss+xml"/><description>Teaching</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Tue, 02 Sep 2025 00:00:00 +0000</lastBuildDate><image><url>https://borja-perez-diaz.github.io/media/icon_hu7729264130191091259.png</url><title>Teaching</title><link>https://borja-perez-diaz.github.io/teaching/</link></image><item><title>Astrophysics and Cosmology</title><link>https://borja-perez-diaz.github.io/teaching/aac/</link><pubDate>Tue, 02 Sep 2025 00:00:00 +0000</pubDate><guid>https://borja-perez-diaz.github.io/teaching/aac/</guid><description>&lt;div class="flex px-4 py-3 mb-6 rounded-md bg-yellow-100 dark:bg-yellow-900">
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&lt;span class="dark:text-neutral-300">Uncompleted Handnotes: the following handnotes are being completed in a slow but continuous way, please be patient.&lt;/span>
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&lt;span class="dark:text-neutral-300">The following handnotes were originally taken in 2013/14 from Prof. Lysiane Mornas and Prof. Luigi Toffolatti. The writter (Dr. Borja Pérez-Díaz) takes fully responsability on the content provided, scientific rigor and updated references.&lt;/span>
&lt;/div>
&lt;p>&lt;strong>INDEX&lt;/strong>&lt;/p>
&lt;ul>
&lt;li>
&lt;p>&lt;a href="https://borja-perez-diaz.github.io/teaching/aac/parti/" target="_blank" rel="noopener">Part I. The Observable in Astrophysics&lt;/a>&lt;/p>
&lt;ul>
&lt;li>&lt;a href="https://borja-perez-diaz.github.io/teaching/aac/parti/1_what_is_astrophysics/" target="_blank" rel="noopener">1. Introduction to astrophysics and cosmology&lt;/a>&lt;/li>
&lt;li>&lt;a href="https://borja-perez-diaz.github.io/teaching/aac/parti/2_general_properties_stars/" target="_blank" rel="noopener">2. General properties of stars&lt;/a>&lt;/li>
&lt;li>
&lt;ol start="3">
&lt;li>Zoology of astrophysical objects&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="4">
&lt;li>Emission, absorption and detection of the radiaton&lt;/li>
&lt;/ol>
&lt;/li>
&lt;/ul>
&lt;/li>
&lt;li>
&lt;p>Part II. The Physics of Stars&lt;/p>
&lt;ul>
&lt;li>
&lt;ol start="5">
&lt;li>Structure equations&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="6">
&lt;li>Properties of the stellar matter&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="7">
&lt;li>Solutions to the structure equations&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="8">
&lt;li>Stellar evolution&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="9">
&lt;li>Binary systems with mass transfer&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="10">
&lt;li>Astrosysmology and variable stars&lt;/li>
&lt;/ol>
&lt;/li>
&lt;/ul>
&lt;/li>
&lt;li>
&lt;p>Part III. Galaxies and Active Galactic Nuclei&lt;/p>
&lt;ul>
&lt;li>
&lt;ol start="11">
&lt;li>Galaxies in the Universe&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="12">
&lt;li>Active Galactic Nuclei and other energetic sources&lt;/li>
&lt;/ol>
&lt;/li>
&lt;/ul>
&lt;/li>
&lt;li>
&lt;p>Part IV. Large Scale Structure and Cosmology&lt;/p>
&lt;ul>
&lt;li>
&lt;ol start="13">
&lt;li>Large Scale Structure&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="14">
&lt;li>Statistics of galaxy distributions&lt;/li>
&lt;/ol>
&lt;/li>
&lt;li>
&lt;ol start="15">
&lt;li>Friedman models&lt;/li>
&lt;/ol>
&lt;/li>
&lt;/ul>
&lt;/li>
&lt;li>
&lt;p>Part V. Appendix&lt;/p>
&lt;ul>
&lt;li>A. Measurements of distances&lt;/li>
&lt;li>B. Thermal History of the Universe&lt;/li>
&lt;/ul>
&lt;/li>
&lt;/ul></description></item></channel></rss>