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BEGIN:VEVENT
DTSTART;TZID=Atlantic/Canary:20221020T103000
DTEND;TZID=Atlantic/Canary:20221020T113000
UID:iactalks-1599
X-WR-CALNAME: IAC Talks: Open Astronomy Seminars
X-ORIGINAL-URL: /iactalks/Talks/view/1599
CREATED:2022-10-20T10:30:00+01:00
X-WR-CALDESC: IAC Talks upcomming talks
SUMMARY:Unveiling the evolutionary history of the Magellanic Clouds through
  detection and analysis of stellar over-densities: clusters and streams.
DESCRIPTION:Unveiling the evolutionary history of the Magellanic Clouds thr
 ough detection and analysis of stellar over-densities: clusters and stream
 s.\nDr. Massimiliano Gatto\n\nThe Magellanic Clouds (MCs) are the closest 
 example of a three-bodyinteracting system composed of the Milky Way (MW), 
 the Large Magellanic Cloud(LMC), and the Small Magellanic Cloud (SMC). The
 refore, the unique opportunityprovided by their relative proximity allowed
  us to analyse with matchless detailthe dynamical and morphological evolut
 ion that a galaxy experience as aconsequence of the mutual gravitational i
 nteraction with its neighbors. In thiscontext, we performed a multi-facete
 d analysis, taking advantage of astrometric,kinematics, and photometric da
 ta, with the main goal of unveiling the pastevolutionary path of the MCs a
 nd their intense interaction history. We tackledthis task by using two com
 plementary approaches: (i) we adopted the propertiesof the MCs star cluste
 r (SC) system to get insights into their past evolutionand (ii) we probed 
 the low-luminous regime of the outer regions of the MCs asthey are the mos
 t sensitive to recent or past tidal stripping events. I willdiscuss the ma
 in outcomes up-to-date of this project and its future perspectivesin light
  of the new ongoing facilities.\nZoom link: https://rediris.zoom.us/j
 /81617686828?pwd=YUpBMXpobUpnYzlpUzluTGo1N2hRQT09\nMeeing ID: 816 1768 682
 8\n Passcode: 990310\nhttps://youtu.be/q1b98yBliFQ\n
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