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VERSION:2.0
CALSCALE:GREGORIAN
PRODID:UW-Madison-Physics-Events
BEGIN:VEVENT
SEQUENCE:0
UID:UW-Physics-Event-4547
DTSTART:20170518T203000Z
DTEND:20170518T220000Z
DTSTAMP:20260419T022532Z
LAST-MODIFIED:20170516T124621Z
LOCATION:4421 Sterling Hall\, Coffee and cookies 3:30 PM\, Talk starts
  at 3:45 PM
SUMMARY:Deep spectroscopy in nearby galaxy clusters: the cases of A85 
 and Hercules clusters\, Astronomy Colloquium\, Alfonso Aguerri\, Titul
 ar OPI en Instituto de Astrofísica de Canarias - ?Instituto de Astrof
 ísica de Canarias
DESCRIPTION:Deep spectroscopical studies in nearby galaxy clusters are
  not frequent in the literature. <br>
\nWe have started a project in o
 rder to obtain deep spectroscopic observations of galaxies in an stati
 stically <br>
\nsignificant sample of nearby galaxy clusters (z < 0.04
 ). This study will provide us spectroscopic properties <br>
\nof galax
 ies in clusters down to M*+6. The kinematics\, stellar population and 
 orbital properties of several <br>
\nthousands of dwarf galaxies in cl
 usters will be analyzed in this survey. In this talk I will show the f
 irst <br>
\nresults on two different nearby clusters: A85 and the Herc
 ules cluster (A2151). These two clusters are massive <br>
\nbut in dif
 ferent dynamical state. I will show the results obtained about the spe
 ctroscopic luminosity functions\, <br>
\nthe orbital analysis of their
  galaxies and the properties of the different types of galaxies spectr
 oscopically selected. 
URL:https://www.physics.wisc.edu/events/?id=4547
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