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<p><span style="font-size: 12pt;"> </span><br>
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<p><span class="contextualExtensionHighlight ms-font-color-themePrimary ms-border-color-themePrimary ident_5_102" tabindex="0" style="font-family:Arial,Helvetica,sans-serif; font-size:12pt; color:rgb(0,0,0)">On Friday the 11th we have the next astronomy seminar
with</span><span style="color:rgb(0,0,0); font-family:Arial,Helvetica,sans-serif; font-size:12pt; white-space:pre-wrap"> </span><span style="font-size:12pt; font-family:Arial,Helvetica,sans-serif; color:rgb(0,0,0)">Anke Arentsen (</span><span style="color:rgb(0,0,0); font-family:Arial,Helvetica,sans-serif; font-size:12pt; white-space:pre-wrap">Observatoire
Astronomique de Strasbourg) </span><span style="font-family:Arial,Helvetica,sans-serif; font-size:12pt">speaking at 10:30 via Zoom.</span></p>
<p><span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px"><b><br>
</b></span></p>
<p><span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px"><b>Galactic Archaeology with the oldest stars in the Milky Way</b></span><br style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">
<br style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">
<span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">The oldest, most metal-poor stars we find in the Milky Way today were born in pristine environments
in the early Universe. They contain unique clues about the First Stars and the early formation and evolution of our Galaxy. Most metal-poor stars are found in the Galactic halo, but the central halo overlapping with the Galactic bulge has often been avoided
— it is challenging to identify metal-poor stars in this dusty, crowded area of the sky. In this talk, I will introduce the Pristine Inner Galaxy Survey (PIGS) which has reached unprecedented efficiency in finding very metal-poor stars in the Galactic bulge
region. I will present recent PIGS results on the chemistry and the kinematics the metal-poor inner Galaxy, and discuss what they can teach us about this ancient component of the Milky Way. Of particular interest in Galactic Archaeology are the carbon-enhanced
metal-poor (CEMP) stars, which are thought to be probes of the First Stars, early chemical evolution and binary interactions. I will also present some recent results on these CEMP stars. </span><br>
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If anyone is interested in chatting with the speaker, we can leave the zoom call opened after the seminar. </div>
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Cheers,</div>
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Chris and Carolina</div>
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<p>Carolina Robustini is inviting you to a scheduled Zoom meeting.</p>
<p><br>
</p>
<p>Topic: Astronomy Department Seminar - Anke Arentsen</p>
<p>Time: Feb 11, 2022 10:30 AM Stockholm</p>
<p><br>
</p>
<p>Join Zoom Meeting</p>
<p>https://stockholmuniversity.zoom.us/j/66310610960?pwd=SitJZGI3ZUl5b3ZzWkNVZEZ1clpmdz09</p>
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<p>Meeting ID: 663 1061 0960</p>
<p>Passcode: 621431</p>
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<p>Join by Skype for Business</p>
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<p><span style="margin:0px; padding:0px; border:0px none; outline:0px; font-size:12.15999984741211px; font-family:Verdana,Arial,Helvetica,sans-serif; vertical-align:baseline; display:block; color:rgb(38,44,42)"><br>
</span><span style="margin:0px; padding:0px; border:0px none; outline:0px; font-size:12.15999984741211px; font-family:Verdana,Arial,Helvetica,sans-serif; vertical-align:baseline; display:block; color:rgb(38,44,42)"></span><span style="margin:0px; padding:0px; border:0px none; outline:0px; vertical-align:baseline; display:block"><span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">Carolina
Robustini </span></span><span style="margin:0px; padding:0px; border:0px none; outline:0px; vertical-align:baseline; display:block"><span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">Inst.
f. Solar Physics, Dept. of Astronomy, Stockholm University</span><br style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">
<span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">AlbaNova University Centre, SE-10691 Stockholm, Sweden</span><br style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont; font-size:13.333333015441895px">
<font color="#212121" face="wf_segoe-ui_normal, Segoe UI, Segoe WP, Tahoma, Arial, sans-serif, serif, EmojiFont" size="2"><span style="">Email: carolina.robustini@astro.su.se</span></font><br>
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