<html>
<head>
<meta http-equiv="Content-Type" content="text/html; charset=iso-8859-1">
<style type="text/css" style="display:none;"> P {margin-top:0;margin-bottom:0;} </style>
</head>
<body dir="ltr">
<div>Hi Everyone,</div>
<div class="elementToProof"><br>
</div>
<div class="elementToProof">This week's lunch talk will be given by Harley, at 1pm on Thursday in A113. Title and abstract are below:</div>
<div class="elementToProof"><br>
</div>
<p class="elementToProof"><span style="font-family: "Aptos", sans-serif; font-size: 12pt; color: black;"><b>Origins of Intracluster Light (in Simulations)</b></span></p>
<p class="elementToProof"><span style="font-family: "Aptos Display", sans-serif; font-size: 12pt; color: rgb(0, 0, 0);"><i> </i></span></p>
<p class="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>
<div class="elementToProof"><br>
</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Thanks,</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Mikey</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div id="Signature" class="elementToProof" style="color: inherit;">
<div style="font-family: Calibri, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(118, 62, 155);">
<b>Mikey Anderson Jennings</b></div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(118, 62, 155);">
<b>Astronomy PhD Student </b></div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<b>University of Nottingham</b></div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<b>Centre for Astronomy and Particle Theory<br>
<br>
</b></div>
</div>
</body>
</html>