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<div dir="ltr">Hi everyone, <span></span></div>
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<div dir="ltr">Reminder of the lunch talk today at 1pm in A113. </div>
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<div dir="ltr">Thanks, </div>
<div dir="ltr">Mikey </div>
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Sent from <a href="https://aka.ms/o0ukef">Outlook for iOS</a></div>
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<div id="divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" style="font-size:11pt" color="#000000"><b>From:</b> Michael Anderson Jennings<br>
<b>Sent:</b> Monday, March 17, 2025 10:49:35 AM<br>
<b>To:</b> astro@nottingham.ac.uk <astro@nottingham.ac.uk><br>
<b>Subject:</b> Lunch Talk</font>
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<div>Hi Everyone,</div>
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<div class="x_elementToProof">This week's lunch talk will be given by Harley, at 1pm on Thursday in A113. Title and abstract are below:</div>
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<p class="x_elementToProof"><span style="font-family:"Aptos",sans-serif; font-size:12pt; color:black"><b>Origins of Intracluster Light (in Simulations)</b></span></p>
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<p class="x_elementToProof"><span style="font-family:"Aptos Display",sans-serif; font-size:12pt; color:black"><i>Despite noteworthy differences between the simulation codes used (and a number of significant differences between the predictions of the two simulations),
the result that roughly Milky-Way mass galaxies are the most significant contributors of ICL stars to halo mass ~ 10<sup>14</sup> M<sub>sun</sub> galaxy clusters at z=0 appears broadly consistent between the two simulations. However, the two simulations do
differ in regards to the predicted significance of secondary ICL formation channels - namely, extra-galactic star-formation in clusters ("in-situ" ICL).</i></span></p>
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Thanks,</div>
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Mikey</div>
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<b>Mikey Anderson Jennings</b></div>
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<b>Astronomy PhD Student </b></div>
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<b>University of Nottingham</b></div>
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<b>Centre for Astronomy and Particle Theory<br>
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