<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 id="divtagdefaultwrapper" style="font-size:12pt;color:#000000;font-family:Calibri,Helvetica,sans-serif;" dir="ltr">
<p><span style="font-family: Helvetica; font-size: 14px;">Dear all,</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">On Friday the 28th of February we have the next Astronomy seminar in room FC61 at 10:30</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Our speaker is Katryn Krekel from the University of Heidelberg.</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Title: Mapping the ionized ISM in nearby galaxies</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Abstract: The ionized interstellar medium (ISM) provides crucial insights into understanding baryon cycling within disk galaxies and tracing radiative and mechanical feedback from young massive stars. With
new VLT/MUSE optical integral field spectroscopy, the PHANGS team now has a wealth of emission line maps that trace different ionization sources and physical conditions across nearby disk galaxies at the 50pc spatial scales needed to isolate individual ionized
regions (e.g. HII regions, supernova remnants, planetary nebulae) from surrounding diffuse ionized gas. I will present our most recent results connecting the molecular gas with observed sites of massive star formation, and measuring the gas phase oxygen abundances
across thousands of HII regions. Within the context of the large scale galactic environment, these studies have implications for our understanding of how spiral structure acts to organize and mix the ISM, and regulate star formation.</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">https://www.albanova.se/event/astronomy-seminar-kathryn-kreckel/</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Upcoming events:</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">28/02 (Fri) @ 10:30: Kathryn Kreckel (MPIA and ARI, Heidelberg)</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">06/03 (Fri) @ 10:30: Leonardo Tartaglia (SU)</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">13/03 (Fri) @ 10:30: Hannah Schunker (MPS, Göttingen)</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">20/03 (Fri) @ 10:30: Svetlana Berdyugina (Freiburg)</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">27/03 (Fri) @ 10:30: TBD</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Kind Regards,</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Arjan and Cristina</span><br style="font-family: Helvetica; font-size: 14px;">
</p>
<p><br>
</p>
<p><span style="font-family: Helvetica; font-size: 14px;">-------------------------------------------</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Dr. Arjan Bik</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Stockholm University</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">AlbaNova University Center</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Department of Astronomy</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">SE-106 91 Stockholm - Sweden</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">Tel: +46 (0) 85537 8549</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">https://www.su.se/english/profiles/abik</span><br style="font-family: Helvetica; font-size: 14px;">
<span style="font-family: Helvetica; font-size: 14px;">-------------------------------------------</span><br style="font-family: Helvetica; font-size: 14px;">
<br style="font-family: Helvetica; font-size: 14px;">
</p>
</div>
</body>
</html>