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Hi Everyone,</div>
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We just wanted to remind you about today's seminar in A113 with Dr. Francesca Frankoudi (Durham). See you all then!</div>
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Kind regards,</div>
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Jesse and Luke</div>
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<div id="divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" style="font-size:11pt" color="#000000"><b>From:</b> Jesse Golden-Marx (staff)<br>
<b>Sent:</b> Monday, June 2, 2025 8:17 AM<br>
<b>To:</b> capt@nottingham.ac.uk <capt@nottingham.ac.uk><br>
<b>Subject:</b> Seminar 4/6/25: Dr. Francesca Frankoudi </font>
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Hi Everyone,</div>
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We just wanted to share the information for this week's seminar with Dr. Francesca Frankoudi (Durham). Francesca will be arriving around 13:30-14:00, so unfortunately, there will not be lunch with the speaker this week. Also, please note that this seminar
is in A113, not C4. The schedule of events is as follows:</div>
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~13:30 - 14:00 -- Arrival</div>
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15:00 - 15:30 -- Meeting with the postgraduate students</div>
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15:45 - 16:45 seminar </div>
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16:45 — Wine and Cheese (in CAPT lobby).</div>
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If you are interested in chatting with Francesca before the seminar, please let us know. </div>
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The title and abstract for Francesca's seminar is given below. See you all on Wednesday.</div>
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Cheers,</div>
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Jesse and Luke</div>
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<span style="font-family:"Aptos Display",sans-serif; font-size:12pt; color:black"><i>The formation, evolution, and dark matter content of barred galaxies in LCDM</i></span></p>
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<span style="font-family:"Aptos Display",sans-serif; font-size:12pt; color:black"><i> </i></span></p>
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<span style="font-family:Aptos,sans-serif; font-size:11pt; color:black">The advent of high resolution hydrodynamical cosmological simulations allows us to now study the internal dynamics of barred spiral galaxies -- such as our own Milky Way -- within the full
ËCDM cosmological context. I will present what we have learnt about the formation and evolution of barred galaxies by comparing cosmological simulations to observations of both the Milky Way and nearby spiral galaxies. In particular, I will address the "When?"
and the "How?" of bar formation in ËCDM, and discuss what this implies about our own Galaxy's formation history, as well as why some galaxies form bars and others don't. I will discuss how barred galaxies evolve throughout cosmic history, as well as the connection
between bars and their host dark matter halos, which can help shed light on both the amount and the nature of dark matter.</span></p>
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<b>Jesse Golden-Marx, Ph.D.</b></div>
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<b>Senior Research Associate</b></div>
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Centre for Astronomy & Particle Theory</div>
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School of Physics & Astronomy</div>
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University of Nottingham</div>
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University Park, Nottingham, UK</div>
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