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DTSTART:19700329T010000
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CATEGORIES:nwe22's list
SUMMARY:The Gaseous Features of the Magellanic System - Bi
 -Qing For (U WAustralia)
DTSTART;TZID=Europe/London:20161129T140000
DTEND;TZID=Europe/London:20161129T150000
UID:TALK69358AThttp://talks.cam.ac.uk
URL:http://talks.cam.ac.uk/talk/index/69358
DESCRIPTION:The Magellanic Stream and Leading Arm which origin
 ated from the Magellanic Clouds are spectacular ga
 seous features. They extend for tens of kpcs and s
 pan for ~200 degree in the southern sky. The close
  proximity of the Magellanic Clouds to the Milky W
 ay provides an excellent opportunity to study inte
 racting galaxy system. I will give an overview of 
 the current research studies on the Magellanic Clo
 uds in various wavelengths and present the results
  of a study of High-Velocity Clouds (HVCs) in the 
 Magellanic Stream and the Leading Arm. The propert
 ies of HVCs in the two regions are compared and co
 ntrasted in order to study the different mechanism
 s shaping their structure and evolution. I will al
 so present potential studies using Australia SKA P
 athfinder.
LOCATION:Ryle Large Meeting Room\, Kavli Building
CONTACT:Neil Wyn Evans
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