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ASKAP and APEX together reveal gas outflow in the Small Magellanic Cloud

26/2/2020

By Enrico Di Teodoro <enrico.diteodoro@gmail.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.

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Mike Ireland is the Australian representative on the ESO Science Technical Committee. He can be reached at michael.ireland@anu.edu.au

Caroline Foster is the Australian representative on the ESO Users Committee. She can be reached at caroline.foster@sydney.edu.au

Stuart Ryder is a Program Manager with AAL. He can be contacted at Stuart.Ryder@astronomyaustralia.org.au

Guest posts are also welcome - please submit these to eso-forum@astronomyaustralia.org.au

ASKAP and APEX together reveal gas outflow in the Small Magellanic Cloud

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