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VERSION:2.0
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METHOD:PUBLISH
BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20091020T000000
DTEND;TZID=Atlantic/Canary:20091020T010000
UID:iactalks-92
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/92
CREATED:2009-10-20T00:00:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Star clusters in M33
DESCRIPTION:Star clusters in M33\nMiss Izaskun San Roman\n\nΛCDM-bas
 ed numerical simulations predict a scenario consistent with observational 
 evidence in Milky Way-like halos. However, less clear is the role of low-m
 ass galaxies in the big picture. The best way to answer this question is t
 o study the nearest example of a dwarf spiral galaxy, M33. We will use sta
 r clusters to understand the structure, kinematics and stellar populations
  of this galaxy. We will present our current status and future plans of a 
 comprehensive study of the star cluster system of M33. This study will pro
 vide key insights into the star formation history, composition and kinemat
 ics of low-mass galaxies as well as place M33 within the context of galaxy
  formation process. 
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