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<p style="font-family:Calibri,sans-serif;margin:0" class="ContentPasted0">Dear Colleague, </p>
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<p style="font-family:Calibri,sans-serif;margin:0" class="ContentPasted0">I am writing to announce the conference “New Views on Feedback and the Baryon Cycle in Galaxies” that we intend to take place in Healesville (Victoria, Australia) from 17-21 July 2023.
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<p style="font-family:Calibri,sans-serif;margin:0" class="ContentPasted0">This is the first call for abstracts for talks and a limited number of posters/short talks. The meeting is limited to 80 people and will take place on a resort in the beautiful Yarra
Valley wine region. This is located roughly an hour outside of Melbourne, Australia. The abstract deadline is
<b class="ContentPasted0">March 15</b>. </p>
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<p style="font-family:Calibri,sans-serif;margin:0" class="ContentPasted0">Please see more information and find abstract submission information at the website: </p>
<p style="font-family:Calibri,sans-serif;margin:0"><a href="https://protect-au.mimecast.com/s/SiXSC2xMQzik95y7jinXOik?domain=outflows2023.com/" target="_blank" rel="noopener noreferrer" data-auth="NotApplicable" data-safelink="true" data-linkindex="0" class="ContentPasted0">https://outflows2023.com/</a></p>
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<p style="font-family:Calibri,sans-serif;margin:0"><u class="ContentPasted0 ContentPasted1">Rationale</u><br class="ContentPasted0 ContentPasted1">
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A consensus exists that the cycle of gas into and out of galaxies is a key aspect regulating star formation and galaxy growth across the history of the Universe. The balance of outflows and accretion are critical aspects of galaxy evolution, and the drivers
whether from stellar evolution or AGN are now necessary to build accurate models of galaxy evolution.
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We aim to bring together a community of researchers in radio, UV, optical and simulations who are studying the diffuse gas around galaxies, and the feedback mechanisms within galaxies that drive the gas flows. We aim to highlight new results on outflows, accretion
and the CGM enabled by pioneering new imaging techniques using ALMA & MUSE/KCWI image slicers and compare these results to the findings of large absorption line studies that have driven the past decades of insights on the baryon cycle. </p>
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<p style="font-family:Calibri,sans-serif;margin:0"><u class="ContentPasted0 ContentPasted1">Current list of Confirmed Speakers: </u></p>
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Lucia Armillotta (Princeton University)</p>
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<span style="background-color: white;" class="ContentPasted0">Danielle Berg (University of Texas)</span><br class="ContentPasted0 ContentPasted1">
Alberto Bolatto (University of Maryland) <br>
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Barbara Catinella (University of Western Australia)<br>
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John Chisholm (University of Texas) </div>
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Rebecca Davies (Swinburne University) </p>
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Drummond Fielding (Flatiron Institute) </p>
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Mark Krumholz (Australia National University) </p>
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Roberto Maiolino (University of Cambridge) </p>
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Anna McLeod (Durham University) <br>
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Emma Ryan - Weber (Swinburne University)<br>
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Evan Schneider (University of Pittsburgh) <br class="ContentPasted0 ContentPasted1">
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Enrico Di Teodoro (University of Florence)</p>
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<div style="color: black; background-color: white;"><span style="background-color: white;"><span class="ContentPasted0 ContentPasted1">Cheers,
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<div class="ContentPasted0 ContentPasted1">Deanne Fisher<br class="ContentPasted0 ContentPasted1">
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on behalf of the SOC (Thorsten Naab, Annalisa Pillipech, Celine Peroux, Fillipo Fraternalli, Luca Cortese, Rebecca Davies)<br class="ContentPasted0 ContentPasted1">
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<div>A.Prof Deanne B. Fisher</div>
<div>ARC Future Fellow</div>
<div>Astro3D Centre of Excellence (CI) Project Lead<br>
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<div>Centre for Astrophysics and Supercomputing</div>
<div>Swinburne University</div>
<div>Phone: +61 39214 4996</div>
<div>email: dfisher@swin.edu.au</div>
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web: deannefisher.com<br>
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