<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Interstellar Medium | James R. Beattie</title><link>https://astro-beattie.com/tags/interstellar-medium/</link><atom:link href="https://astro-beattie.com/tags/interstellar-medium/index.xml" rel="self" type="application/rss+xml"/><description>Interstellar Medium</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Wed, 03 Jun 2026 00:00:00 +0000</lastBuildDate><image><url>https://astro-beattie.com/media/icon_hu58f049e2f3dec21651e29209817604b1_360074_512x512_fill_lanczos_center_3.png</url><title>Interstellar Medium</title><link>https://astro-beattie.com/tags/interstellar-medium/</link></image><item><title>My single-author ApJL paper on supernova-driven turbulence</title><link>https://astro-beattie.com/post/supernova-turbulence-apjl/</link><pubDate>Wed, 03 Jun 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/post/supernova-turbulence-apjl/</guid><description>&lt;p>My single-author paper, &lt;em>Supernovae Drive Large-scale, Incompressible Turbulence through Small-scale Instabilities&lt;/em>, is published in &lt;a href="https://doi.org/10.3847/2041-8213/ae6eed">The Astrophysical Journal Letters, 1004, L9&lt;/a>.&lt;/p>
&lt;p>I study how individual supernova remnants generate incompressible turbulence. Instabilities wrinkle the interface between hot and warm gas, bringing pressure and density gradients out of alignment and generating vorticity. Vortex stretching then allows turbulent motions to escape the shell into the surrounding gas.&lt;/p>
&lt;p>The result connects the structure of these thin interfaces to the wider galactic turbulence cascade: small-scale instabilities can supply turbulent motions that an inverse cascade carries to larger scales. Sections III and IV of the &lt;a href="https://arxiv.org/html/2509.07354v4">paper&lt;/a> develop and test this mechanism.&lt;/p>
&lt;p>&lt;a href="https://doi.org/10.3847/2041-8213/ae6eed">Read the published paper&lt;/a>, &lt;a href="https://arxiv.org/abs/2509.07354">read the open preprint&lt;/a>, or &lt;a href="https://astro-beattie.com/publication/sne_turbulence_baroclinic/">explore the science highlight&lt;/a>.&lt;/p></description></item><item><title>Matt Sampson’s cosmic-ray study is published</title><link>https://astro-beattie.com/post/cr-coupling-published/</link><pubDate>Wed, 08 Apr 2026 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/post/cr-coupling-published/</guid><description>&lt;p>Our study, &lt;em>Cosmic-Ray and Plasma Coupling for Isothermal Supersonic Turbulence in the Magnetized Interstellar Medium&lt;/em>, led by Matt Sampson, is now published in &lt;em>The Astrophysical Journal&lt;/em>, volume 1001, article 99 (April 2026).&lt;/p>
&lt;p>The paper explores how cosmic rays and turbulent, magnetized plasma interact as the cosmic-ray diffusion and streaming properties vary. Congratulations, Matt, and thank you to all our collaborators!&lt;/p>
&lt;p>&lt;a href="https://doi.org/10.3847/1538-4357/ae4edc">Read the published paper&lt;/a> or &lt;a href="https://arxiv.org/abs/2506.03768">read the preprint&lt;/a>.&lt;/p></description></item><item><title>Matt Sampson’s cosmic-ray and plasma-coupling study is on arXiv</title><link>https://astro-beattie.com/post/cr_coupling_arxiv/</link><pubDate>Wed, 04 Jun 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/post/cr_coupling_arxiv/</guid><description>&lt;p>Our study of cosmic-ray and plasma coupling, led by Matt Sampson, is available as a &lt;a href="https://arxiv.org/abs/2506.03768">preprint on arXiv&lt;/a>.&lt;/p>
&lt;p>&lt;strong>Update, April 2026:&lt;/strong> The paper is now &lt;a href="https://astro-beattie.com/post/cr-coupling-published/">published in The Astrophysical Journal&lt;/a>.&lt;/p></description></item><item><title>🎉Congrats Neco Kriel🎉 (ANU) -- student-led study published on the supersonic turbulent dynamo!</title><link>https://astro-beattie.com/post/compressible_dynamo_published/</link><pubDate>Fri, 31 Jan 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/post/compressible_dynamo_published/</guid><description/></item><item><title>Fundamental MHD scales -- II: the kinematic phase of the supersonic small-scale dynamo</title><link>https://astro-beattie.com/publication/fundamental_scales_2/</link><pubDate>Fri, 31 Jan 2025 00:00:00 +0000</pubDate><guid>https://astro-beattie.com/publication/fundamental_scales_2/</guid><description>&lt;!-- This work is driven by the results in my [previous paper](/publication/conference-paper/) on LLMs.
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