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PRODID:UW-Madison-Physics-Events
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UID:UW-Physics-Event-4473
DTSTART:20170209T213000Z
DTEND:20170209T110000Z
DTSTAMP:20260419T042734Z
LAST-MODIFIED:20170131T143005Z
LOCATION:4421 Sterling Hall\, Coffee and Cookies 3:30 pm. Talk Begins 
 3:45 PM
SUMMARY:Insights into Galaxies using Dynamical Modeling\, Astronomy Co
 lloquium\, Shravan Shetty\, UW Madison Astronomy Department
DESCRIPTION:Understanding the underlying mass distribution of galaxies
  promises to unveil immense information about galaxies\, however conve
 rting their observed two dimensional kinematics into three dimensional
  mass distributions is a degenerate problem. Various techniques have b
 een used to create the detailed dynamical models of galaxies but the m
 ost general and reliable of these techniques tend to be computationall
 y intensive even today and hence are applicable to only small number o
 f galaxies. In recent years however\, based on empirical results\, the
  Jeans Anisotropic Models (JAM) have allowed astronomers to create det
 ailed dynamical models for large number of galaxies. Using this techni
 que\, I present the results of my PhD thesis wherein I study the<br>
\
 nevolution of galaxies with redshift and with environment. 
URL:https://www.physics.wisc.edu/events/?id=4473
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