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Understanding the gas dynamics in the central 3 kpc of the Milky Way

September 7, 2018
From 10:30 until 12:00

Mattia Sormani

Heidelberg

I give an introduction to the gas dynamics in the bar region of the Milky Way, which is characterised by strong non-circular motions. I show how this allows to interpret the observed CO and HI longitude-velocity maps in the region l < |30| degrees.

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