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PRODID:UW-Madison-Physics-Events
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UID:UW-Physics-Event-6389
DTSTART:20210401T203000Z
DTEND:20210401T220000Z
DTSTAMP:20260414T234209Z
LAST-MODIFIED:20210311T180433Z
LOCATION:Zoom meeting(see Abstract ) Coffee and tea 3:30pm\, Talk 3:45
 pm
SUMMARY:How do galaxies in the nearby Universe grow?\, Astronomy Collo
 quium\, Sanchayeeta Borthakur\,\, Arizona State
DESCRIPTION:Galaxy growth is a slow but continuous process. The observ
 ed properties of galaxies suggest that accretion must continue to supp
 ort star formation. However\, direct observational evidence of gas flo
 ws into galaxies have been extremely hard to come by. One of the most 
 promising regions in our search has been the disk-halo interface\, whe
 re we are uncovering signs of gas condensation.<br>
\n<br>
\nIn this t
 alk\, I will discuss the results from our ongoing DIISC (Deciphering t
 he Interplay between the ISM\, Stars\, and the CGM) survey\, which pro
 bes the disk-halo interface. I'll discuss our findings in terms of the
  signpost of gas accretion and galactic feedback. I'll also show evide
 nce that structures such as high-velocity clouds and extra-planar gas 
 seen in the Milky Way and a few other galaxies are indeed prevalent in
  most galaxies. These gaseous structures represent a pathway for gas a
 ccretion into galaxies and can be one of the primary ways how galaxies
  accrete gas in the nearby Universe.<br>
\nZoom Link<br>
\nhttps://uwm
 adison.zoom.us/j/88513896776?pwd=Y1JtRE1KZllxWkFTamJBSGtGdm9yQT09<br>

 \n
URL:https://www.physics.wisc.edu/events/?id=6389
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