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Largest ALMA ever image shows hidden chemistry at the heart of the Milky Way
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The cold gas across the central molecular zone of the Milky Way, a region that stretches out to about 650 light-years, has been explored in such detail for the first time.
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ICE-CSIC is part of the ALMA CMZ Exploration Survey (ACES), which specifically explores cold molecular gas, aiming to better understand star formation.
Largest ALMA image ever shows the molecular gas in the centre of the Milky Way. Credits: ALMA(ESO/NAOJ/NRAO)/S. Longmore et al. Background: ESO/D. Minniti et al.
A striking new image captures the central region of our Milky Way, unveiling a complex network of filaments of cosmic gas in unprecedented detail. Obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), this rich dataset will allow astronomers to probe the lives of stars in the most extreme region of our galaxy, next to the supermassive black hole at its centre. The research, in which the Institute of Space Sciences (ICE-CSIC) is involved, is published today in a series of papers in the Monthly Notices of the Royal Astronomical Society.
“It’s a place of extremes, invisible to our eyes, but now revealed in extraordinary detail,” says Ashley Barnes, an astronomer at the European Southern Observatory (ESO) in Germany who is part of the team that obtained the new data. The observations provide a unique view of the cold gas — the raw material from which stars form — within the so-called Central Molecular Zone (CMZ) of our galaxy. It is the first time the cold gas across this whole region has been explored in such detail.
The region featured in the new image spans more than 650 light-years. It harbours dense clouds of gas and dust, surrounding the supermassive black hole at the centre of our galaxy. “It is the only galactic nucleus close enough to Earth for us to study in such fine detail,” says Barnes. The dataset reveals the CMZ like never before, from gas structures dozens of light-years across all the way down to small gas clouds around individual stars.
The gas that ACES — the ALMA CMZ Exploration Survey — specifically explores is cold molecular gas. The survey unpacks the intricate chemistry of the CMZ, detecting dozens of different molecules, from simple ones such as silicon monoxide to more complex organic ones like methanol, acetone or ethanol.
Cold molecular gas flows along filaments feeding into clumps of matter out of which stars can grow. In the outskirts of the Milky Way we know how this process happens, but within the central region the events are much more extreme. “The CMZ hosts some of the most massive stars known in our galaxy, many of which live fast and die young, ending their lives in powerful supernova explosions, and even hypernovae,” says ACES leader Steve Longmore, a professor of astrophysics at Liverpool John Moores University, UK. With ACES, astronomers hope to better understand how these phenomena influence the birth of stars and whether our theories of star formation hold in extreme environments.
“Previously, it was only feasible to study a limited number of regions within the CMZ in such a high level of detail. Now, the large mosaic of the entire CMZ obtained by the ACES team opens the door to a new realm of unexpected findings and surprises. Gaining a deeper understanding of this significant part of our galaxy with this level of detail will also enable us to better comprehend analogous regions in distant galaxies distributed throughout the entire Universe”, says Álvaro Sánchez-Monge, ICE-CSIC researcher affiliated to the Institute of Space Sciences of Catalonia (IEEC).
Star formation in the central region of the Milky Way
To collect this new dataset, astronomers used ALMA, which is operated by ESO and partners in Chile’s Atacama Desert. This is the first time such a large area has been scanned with this facility, making this the largest ALMA image ever. In the sky, the mosaic — obtained by stitching together many individual observations like putting puzzle pieces together — is as long as three full moons side-by-side.
“We anticipated a high level of detail when designing the survey, but we were genuinely surprised by the complexity and richness revealed in the final mosaic," says Katharina Immer, an ALMA astronomer at ESO who is also part of the project.
“The upcoming ALMA Wideband Sensitivity Upgrade, along with ESO’s Extremely Large Telescope, will soon allow us to push even deeper into this region — resolving finer structures, tracing more complex chemistry, and exploring the interplay between stars, gas and black holes with unprecedented clarity,” says Barnes. “In many ways, this is just the beginning.”
More information
This research was presented in a series of papers presenting the ACES data, to appear in Monthly Notices of the Royal Astronomical Society.
The data itself will be available from the ALMA Science Portal at: https://almascience.org/alma-data/lp/aces