This image shows the location of the Central Molecular Zone (CMZ), a region at the core of our galaxy rich in dense and intricate gas clouds. This zone has been mapped with the Atacama Large Millimeter/submillimeter Array (ALMA), as part of the ALMA CMZ Exploration Survey or ACES. The inset is an ACES image where different molecules are displayed in different colours. The entire image – the largest ever made with ALMA – is as long as three full Moons side-by-side in the sky. Credit: ALMA(ESO/ NAOJ/ NRAO)/ S Longmore et al. Stars in inset: ESO/ D Minniti et al. Milky Way: ESO/ S Guisard.
In the largest image of its kind to date, hidden chemistry at the heart of the Milky Way has been shown to exist.
Astronomers have captured the central region of our Milky Way in a striking new image, unveiling a complex network of filaments of cosmic gas in unprecedented detail.
Obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), this rich dataset — the largest ALMA image to date — 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.
Ashley Barnes, an astronomer at the European Southern Observatory (ESO) in Germany who is part of the team that obtained the new data, said: “It’s a place of extremes, invisible to our eyes, but now revealed in extraordinary detail.”
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.
Barnes said: “It is the only galactic nucleus close enough to Earth for us to study in such fine detail.”
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.
This image shows the complex distribution of molecular gas in the Central Molecular Zone (CMZ) of the Milky Way. It was obtained with the Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner. This map is as long as three full Moons side-by-side in the sky, and it is in fact the largest ALMA image ever obtained. This map is part of ACES — the ALMA CMZ Exploration Survey — a project designed to understand how gas condenses into stars in the extreme and chaotic environment at the heart of our galaxy. The survey has charted the distribution of dozens of different molecules, five of which are shown here in different colours: sulphur monoxide (cyan), silicon monoxide (green), isocyanic acid (red), cyanoacetylene (blue), and carbon monosulphide (magenta). The stars in the foreground of this image were observed at infrared wavelengths (Y, Z and J filters) with ESO’s VISTA telescope as part of a different project. The actual density of stars in the CMZ is much higher than what is shown here, where we have opted to highlight the details in the molecular cloud. Note that the edges of the ALMA map appear somewhat sharp because the ALMA observations do not cover the entire rectangular area here. Credit: ALMA(ESO/ NAOJ/ NRAO)/ S Longmore et al. Background: ESO/ D Minniti et al.
Intricate chemistry
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.
ACES leader Steve Longmore, a professor of astrophysics at Liverpool John Moores University, UK, said: “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.”
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.
Longmore added: “By studying how stars are born in the CMZ, we can also gain a clearer picture of how galaxies grew and evolved.
“We believe the region shares many features with galaxies in the early Universe, where stars were forming in chaotic, extreme environments.”
Mosaic
To collect this new dataset, astronomers used ALMA, which is operated by ESO and partners in Chile’s Atacama Desert.
In fact, this is the first time such a large area has been scanned with this facility, making this the largest ALMA image ever.
Seen 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.
Katharina Immer, an ALMA astronomer at ESO who is also part of the project, said: “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.”
The data from ACES are presented in five papers accepted for publication in Monthly Notices of the Royal Astronomical Society, with a sixth in the final review stages.
Barnes said: “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.
“In many ways, this is just the beginning.”
