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SUMMARY:The Formation of Magellanic System and the total mass of Large Mag
 ellanic Cloud
DTSTART;VALUE=DATE-TIME:20230322T164500Z
DTEND;VALUE=DATE-TIME:20230322T170000Z
DTSTAMP;VALUE=DATE-TIME:20241114T092443Z
UID:indico-contribution-208@meetings.aip.de
DESCRIPTION:Speakers: Jianling WANG (National Astronomical Observatories\,
  Chinese Academy of Sciences)\nThe Magellanic Stream is unique to sample t
 he MW potential from ~50kpc to 300\nkpc\, and is also unique in constraini
 ng the LMC mass\, an increasingly important\nquestion for the Local Group/
 Milky Way modeling.  I will compare on the\nstrengths and weaknesses of th
 e two types of  models (tidal and ram-pressure) of\nthe Magellanic Stream 
 formation.  I will present our modeling for the formation\nof the Magellan
 ic System\, including those of the most recent discoveries in the\nStream\
 , in the Bridge and at the outskirts of Magellanic Clouds. This model has\
 nbeen successful in predicting most recent observations in both properties
  of\nstellar and gas phase. It appears that it is an over-constrained mode
 l and\nprovides a good path to investigate the Stream properties.  In part
 icular\, this\nmodel requires LMC mass significantly smaller than 10^11 Ms
 un.\n\nhttps://iaus379.aip.de/event/20/contributions/208/
LOCATION:Haus H\, Telegrafenberg
URL:https://iaus379.aip.de/event/20/contributions/208/
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