Astronomers have observed a massive and extremely active barred spiral galaxy in the early Universe and found that it has important similarities and differences with modern galaxies.
This improves our understanding of how barred spiral galaxies, like our own Milky Way Galaxy, grow and evolve.
The team, led by Shuo Huang, a project researcher at the National Astronomical Observatory of Japan and Nagoya University, used the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope to observe a massive barred spiral galaxy known as J0107a that existed 11.1 billion years ago.
Unique patterns of spiral galaxies
Some spiral galaxies, including the Milky Way, exhibit a straight bar inside the spiral pattern. This bar structure helps channel gas towards the galaxy’s centre, where it can be used to form new stars.
However, the reason why bars form in only about half of spiral galaxies and how they influence the evolution of the galaxy are unanswered questions.
Located in the constellation Cetus, J0107a is a “monster” galaxy, meaning a galaxy growing rapidly in the early Universe by forming many new stars.
Due to them being located far away, it has been difficult to see the detailed structure of monster galaxies and determine what is driving this vigorous star formation.
Recently, the improved resolution provided by the James Webb Space Telescope has revealed spirals and even bars in some of the monster galaxies.
J0107a is the earliest and most massive barred spiral galaxy known to date, so it is the best target for studying the evolution of barred spiral galaxies in the early Universe.
Differences compared to modern galaxies
The team found that in J0107a, the distribution and motion of gas in the bar are similar to those of modern galaxies.
However, compared to modern galaxies, the concentrations of gas are several times higher, and the speed of the gas flow is faster, reaching several hundred kilometres per second in spiral galaxies.
Astronomers believe that this massive influx of gas to the centre will fuel significant additional star formation, helping to drive the evolution of this monster galaxy. This is the first time these features have been observed, and they were not predicted by theoretical or simulation models.
Huang commented: “We expect that the detailed information about the distribution and movement of gas gained through these observations will provide important clues for exploring not only the origins of the diversity of galaxies, but also the formation and evolution of more normal barred spiral galaxies.”
