By Enrico Di Teodoro <email@example.com>
Fig. 1: The Small Magellanic Cloud in H-alpha emission (MCELS survey), showing intense star formation across the galaxy. The atomic hydrogen structures where we detected molecular gas with APEX are shown in blue.
The access to ESO facilities is opening up great opportunities of carrying out new exciting research for the astronomy community in Australia. In particular, I have used this opportunity to study local galactic winds.
Michael Murphy is the Australian representative on the ESO Science Technical Committee. He can be reached at firstname.lastname@example.org