AN INTERACTION OF A MAGELLANIC LEADING ARM HIGH-VELOCITY CLOUD WITH THE MILKY WAY DISK

摘要

The Leading Arm of the Magellanic system is a tidally formed H i feature extending ～60° from the Magellanic Clouds ahead of their direction of motion. Using atomic hydrogen (H i) data from the Galactic All-Sky Survey (GASS), supplemented with data from th