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SUMMARY:The Gaseous Features of the Magellanic System - Bi-Qing For (U WAu
 stralia)
DTSTART:20161129T140000Z
DTEND:20161129T150000Z
UID:TALK69358@talks.cam.ac.uk
CONTACT:Neil Wyn Evans
DESCRIPTION:The Magellanic Stream and Leading Arm which originated from th
 e Magellanic Clouds are spectacular gaseous features. They extend for tens
  of kpcs and span for ~200 degree in the southern sky. The close proximity
  of the Magellanic Clouds to the Milky Way provides an excellent opportuni
 ty to study interacting galaxy system. I will give an overview of the curr
 ent research studies on the Magellanic Clouds in various wavelengths and p
 resent the results of a study of High-Velocity Clouds (HVCs) in the Magell
 anic Stream and the Leading Arm. The properties of HVCs in the two regions
  are compared and contrasted in order to study the different mechanisms sh
 aping their structure and evolution. I will also present potential studies
  using Australia SKA Pathfinder.
LOCATION:Ryle Large Meeting Room\, Kavli Building
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