Speaker
Imogen Barnsley
(University of Adelaide)
Description
In this update, we will present preliminary results from our 3D molecular hydrogen distributions of ISM cloud structures, derived over the entire Mopra Southern Galactic Plane CO Survey. We will introduce our novel cloud identification method used to create these distributions. This involves Gaussian decompositions and clustering, as well as combining measurements from different gas tracers (12CO and 13CO).
Author
Imogen Barnsley
(University of Adelaide)