Researchers have discovered the most distant Milky-Way-like galaxy yet observed. Dubbed REBELS-25, this disc galaxy seems as orderly as present-day galaxies, but we see it as it was when the Universe was only 700 million years old. This is surprising since, according to our current understanding of galaxy formation, such early galaxies are expected to appear more chaotic. Leiden astronomers Lucie Rowland and Jacqueline Hodge tell about their discovery.
The galaxies we see today have come a long way from their chaotic, clumpy counterparts that astronomers typically observe in the early Universe. 'According to our understanding of galaxy formation, we expect most early galaxies to be small and messy looking,' says co-author Jacqueline Hodge.
These messy, early galaxies merge with each other and then evolve into smoother shapes at an incredibly slow pace. Current theories suggest that, for a galaxy to be as orderly as our own Milky Way - a rotating disc with tidy structures like spiral arms - billions of years of evolution must have elapsed. The detection of REBELS-25, however, challenges that timescale.
To organized for a young galaxy?
The rotation and structure of REBELS-25 were revealed using the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile, in which the European Southern Observatory (ESO) is a partner. In the study, accepted for publication in Monthly Notices of the Royal Astronomical Society, astronomers found REBELS-25 to be the most distant strongly rotating disc galaxy ever discovered. The light reaching us from this galaxy was emitted when the Universe was only 700 million years old - a mere five percent of its current age (13.8 billion) - making REBELS-25's orderly rotation unexpected.
'Seeing a galaxy with such similarities to our own Milky Way, that is strongly rotation-dominated, challenges our understanding of how quickly galaxies in the early Universe evolve into the orderly galaxies of today's cosmos,' says PhD candidate and first author Lucie Rowland.
'Only ALMA is capable for the job'
REBELS-25 was initially detected in previous observations by the same team, also using ALMA. At the time, it was an exciting discovery, showing hints of rotation, but the resolution of the data was not fine enough to be sure. Therefore, the team performed follow-up observations with ALMA at a higher resolution, which confirmed its record-breaking nature. 'ALMA is the only telescope in existence with the sensitivity and resolution to achieve this,' says co-author Renske Smit, a researcher at Liverpool John Moores University (United Kingdom).
Spiral arms are transforming our understanding
Surprisingly, the data also hinted at more developed features similar to those of the Milky Way, like a central elongated bar, and even spiral arms, although more observations will be needed to confirm this. 'Finding further evidence of more evolved structures would be an exciting discovery, as it would be the most distant galaxy with such structures observed to date,' says Rowland.
These future observations of REBELS-25, alongside other discoveries of early rotating galaxies, will potentially transform our understanding of early galaxy formation, and the evolution of the Universe as a whole.
Read the original press release on the website of ESO.
Collaboration
This research is presented in a paper entitled "REBELS-25: Discovery of a dynamically cold disc galaxy at z=7.31" to appear in Monthly Notices of the Royal Astronomical Society.
The observations were conducted as part of the ALMA Large Program REBELS: Reionization Era Bright Emission Lines Survey.
Reading further
REBELS-25: Discovery of a dynamically cold disc galaxy at z=7.31. Door: Lucie E. Rowland, Jacqueline Hodge, Rychard Bouwens, Pavel Mancera Piña, Alexander Hygate, Hiddo Algera, Manuel Aravena, Rebecca Bowler, Elisabete da Cunha, Pratika Dayal, Andrea Ferrara, Thomas Herard-Demanche, Hanae Inami, Ivana van Leeuwen, Ilse de Looze, Pascal Oesch, Andrea Pallottini, Siân Phillips, Matus Rybak, Sander Schouws, Renske Smit, Laura Sommovigo, Mauro Stefanon & Paul van der Werf. Geaccepteerd voor publicatie in Monthly Notices of the Royal Astronomical Society.
Read the original press release on eso.org.
