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X-WR-CALNAME;VALUE=TEXT:ITC Luncheon 
PRODID:-//Harvard events data//EN
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UID:event_1593091_0
SUMMARY:ITC Luncheon 
DESCRIPTION:<p style="margin-top:0pt;margin-bottom:0pt">	<span style="caret-color:#000000"><span style="color:#000000"><span style='ms",sans-serif'><span style="line-height:1.38"><font face="trebuchet ms, sans-serif"><span style="text-align:center"><strong>Eric Andersson (AMNH) </strong>“</span>Pre-supernovae feedback set the star cluster mass function to a power law"</font></span></span></span></span></p><p style="margin-top:0pt;margin-bottom:0pt">	<span style='ms",sans-serif'><span style="color:#222222"><span style="line-height:1.38"><font face="trebuchet ms, sans-serif"><span style="color:#000000;text-align:center"><strong>Ygal Klein (Weizmann Inst. of Science)</strong> "</span><span style="text-align:center;color:#000000">Complex high e dynamics reduce to simple pendulum models"</span></font></span></span></span></p><p style="margin-top:0pt;margin-bottom:0pt">	<span style='ms",sans-serif'><span style="color:#222222"><span style="line-height:1.38"><font face="trebuchet ms, sans-serif"><span style="color:#000000;text-align:center"><strong>Fengwu Sun (CfA)</strong> "</span><span style="text-align:center;color:#000000">Most of cosmic star formation at redshift 5 is still obscured by dust"</span></font></span></span></span></p><p style="margin-top:0pt;margin-bottom:0pt">	<span style='ms",sans-serif'><span style="color:#222222"><span style="line-height:1.38"><font face="trebuchet ms, sans-serif"><span style="color:#000000;text-align:center"><strong>Justus Gibson (Colorado) </strong>"</span><span style="text-align:center;color:#000000">JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations"</span></font></span></span></span></p>
LOCATION:Phillips Auditorium
STATUS:CONFIRMED
DTSTART:20240919T163000Z
DTEND:20240919T173000Z
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