Largest ALMA image ever shows the molecular gas in the centre of the Milky Way (Credit: ALMA(ESO/NAOJ/NRAO)/S. Longmore et al. Background: ESO/D. Minniti et al.)

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.

“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.

Different molecules in the centre of the Milky Way observed with ALMA: ACES has mapped the distribution of several dozen molecules at the centre of our galaxy. Here we show five of them, from top to bottom: carbon monosulphide, isocyanic acid, silicon monoxide, sulphur monoxide, and cyanoacetylene. (Credit: ALMA(ESO/NAOJ/NRAO)/S. Longmore et al.)

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.

“By studying how stars are born in the CMZ, we can also gain a clearer picture of how galaxies grew and evolved,” Longmore adds. “We believe the region shares many features with galaxies in the early Universe, where stars were forming in chaotic, extreme environments.”

To collect this new dataset, astronomers used ALMA 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. 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.

Xing Lu, a research professor at Shanghai Astronomical Observatory, is a core member of the data reduction working group of the ACES project, and leads one of the data release papers, i.e., Paper IV. In this paper, they release data of the two intermediate-width spectral windows of ACES, including images of six representative molecular lines. In addition, they analyze the morphological similarity between the continuum and a dozen of molecular lines and the line ratios between several pairs of isotologues and isotopomers, and discover the extraordinarily strong SO emission in the Sgr B2 cloud, the potential of using HC15N as a robust tracer of dense molecular gas, and the possibility of using the line ratio between HN13C and H13CN as a thermometer of molecular gas in the CMZ. Several researchers and students from Shanghai Astronomical Observatory have contributed to the ACES project in different working groups. “We are running parallel projects in the K-band to observe key molecular lines to constrain the gas temperature in the ACES field. The Tianma 65-m telescope of Shanghai Astronomical Observatory and its new 7-beam K-band receiver will be crucial part of this effort,” says Xing Lu.

The data from ACES are presented in five papers accepted for publication in Monthly Notices of the Royal Astronomical Society, with a sixth nearing acceptance.

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:

Paper I - ALMA Central Molecular Zone Exploration Survey (ACES) I: Overview paper