First detection of cold, dense gas outflowing from Milky Way's centre
- That the Milky Way has a “galactic wind” — streams of fast particles blowing out from the Galactic Centre
- How researchers detected that parts of this wind are very cold and composed of molecular gas
- Why this outflow of cold gas could affect the future of the Milky Way
After discovering the warm component of the galactic wind, Di Teodoro’s team wanted to go further. "We had often wondered about the possibility of detecting cold molecular gas and the 2017 ESO-Australia agreement finally allowed us to access the unique ESO facilities, including APEX." says Di Teodoro.
APEX is the 12-metre Atacama Pathfinder Experiment (APEX) radio telescope that can observe during the day as well as the night. The team targeted two clouds of gas travelling out from the Galactic Centre — which both contain large quantities of hydrogen atoms — to see if they also contain outflowing cold gas. Using APEX, they searched for carbon monoxide, which is commonly found in cold molecular gas clouds. APEX is well suited to the task, thanks to its high sensitivity and ability to map relatively large regions of the sky.
The team’s observations revealed carbon monoxide emission in both clouds, which intriguingly had very different properties between them. The further out cloud was moving faster and was more diffuse and more turbulent, suggesting that the cold gas was mixing with its surroundings more, perhaps because it has had more time to interact with them. Alternatively, the differences may be caused by local variations in the hot outflow between the locations of the two clouds.
"Our exploratory APEX observations actually surprised us, because we did not expect such a large amount of cold molecular gas, based on our current understanding of galactic winds," explains Di Teodoro.
"Stars are formed from the collapse of giant clouds of molecular gas, which is exactly the same kind of material that we are observing in the Milky Way's outflow. This means that our galaxy is expelling the best fuel to form new stars."
Fresh gas continuously flows from the external regions of the galaxy towards the inner regions and replenishes this fuel reservoir. However, if the amount of gas flowing in is lower than the amount of gas flowing out in the wind, at some point there will be a shortage of fuel and no new stars will be able to form in the inner galaxy.
Di Teodoro continues, "If the galactic wind gets stronger in the future, for example if the supermassive black hole increases its level of activity, then this could affect the entire galaxy."
How such a large amount of cold gas could be moving at high speed in the galactic wind is puzzling. In the central regions of more active galaxies, cool gas can be accelerated by a very active supermassive black hole or when extraordinarily high numbers of stars form in a “starburst” and eject powerful stellar winds, but neither is the case for the Milky Way. Alternatively, fast-moving cool clouds may be formed when the fast-moving hot wind mixes with slow-moving, cool clouds that are not part of the wind.
The APEX telescope, in which ESO is a partner, studies how stars form in our galaxy by observing cold and dusty clouds of molecular gas. By building databases of these large “stellar nurseries”, we can understand how and under what conditions star formation takes place, as well as the large-scale structure of the galaxy. APEX’s location 5100 metres above sea level on the Chajnantor plateau in the dry Atacama Desert in northern Chile provides a unique window to study the Universe in submillimetre light.
This first detection of outflowing cold molecular gas from the centre of the Milky Way challenges our current theories of how galactic winds form and affect the future evolution of our galaxy. More observations of a larger number of molecular gas clouds are needed to provide a more complete picture of their origin.
Numbers in this article
|12||Diameter (in metres) of APEX’s dish|
|2017||Year that the ESO-Australia agreement was signed|
|5100||Height of APEX above sea level|
Biography Emma Foxell
Emma Foxell is a science communication intern at ESO. Before this, she completed her PhD at the University of Warwick (UK) in the field of exoplanets and transit surveys, focusing on red dwarfs.