A galaxy first seen less than 800 million years after the Big Bang, when the universe was less than 6 percent of its current age, is actually a massive galaxy and a smaller neighbor that will soon form an even larger structure.
Astronomers expect that the first galaxies would share many similarities with some of the dwarf galaxies seen in the nearby universe today. These early agglomerations of a few billion stars would then become the building blocks of the larger galaxies that came to dominate the universe after the first few billion years.
However, ongoing observations with the Atacama Large Millimeter/submillimeter Array, or ALMA, discovered surprising examples of massive, star-filled galaxies seen when the cosmos was less than a billion years old.
The findings suggest that smaller galactic building blocks were able to assemble into large galaxies quite quickly.
The most recent ALMA observations push back this epoch of massive-galaxy formation even further by identifying two giant galaxies seen when the universe was only 780 million years old, or about 5 percent its current age. Further, ALMA revealed that these uncommonly large galaxies are nestled inside an even-more-massive cosmic structure, a halo of dark matter several trillion times more massive than the sun.
The two galaxies are in such close proximity—less than the distance from the Earth to the center of our galaxy—that they will shortly merge to form the largest galaxy ever observed at that period in cosmic history.
Assembly in action
As reported in Nature, the discovery provides new details about the emergence of large galaxies and the role that dark matter plays in assembling the most massive structures in the universe.
The larger of the two is forming stars at a rate of 2,900 solar masses per year.
“With these exquisite ALMA observations, astronomers are seeing the most massive galaxy known in the first billion years of the universe in the process of assembling itself,” says lead author Dan Marrone, associate professor of astronomy at the University of Arizona.
Astronomers are seeing these galaxies during a period of cosmic history known as the Epoch of Reionization, when most of intergalactic space was suffused with an obscuring fog of cold hydrogen gas. As more stars and galaxies formed, their energy eventually ionized the hydrogen between the galaxies, revealing the universe as we see it today.
“We usually view that as the time of little galaxies working hard to chew away at the neutral intergalactic medium,” Marrone says. “Mounting observational evidence with ALMA, however, has helped to reshape that story and continues to push back the time at which truly massive galaxies first emerged in the universe.”
The studied galaxies, collectively known as SPT0311-58, originally were identified as a single source by the South Pole Telescope. These first observations indicated that this object was very distant and glowing brightly in infrared light, meaning that it was extremely dusty and likely going through a burst of star formation. Subsequent observations with ALMA revealed the distance and dual nature of the object, clearly resolving the pair of interacting galaxies.
To make this observation, ALMA had some help from a gravitational lens, which provided an observing boost to the telescope. Gravitational lenses form when an intervening massive object, such as a galaxy or galaxy cluster, bends the light from more distant galaxies. They do, however, distort the appearance of the object being studied, requiring sophisticated computer models to reconstruct the image as it would appear in its unaltered state.
This “de-lensing” process provided intriguing details about the galaxies, showing that the larger of the two is forming stars at a rate of 2,900 solar masses per year. It also contains about 270 billion times the mass of our sun in gas and nearly 3 billion times the mass of our sun in dust.
“That’s a whopping large quantity of dust, considering the young age of the system,” says Justin Spilker, a recent graduate of the University of Arizona and now a postdoctoral fellow at the University of Texas, Austin.
The astronomers determined that the galaxy’s rapid star formation was likely triggered by a close encounter with its slightly smaller companion, which already hosts about 35 billion solar masses of stars and is increasing its rate of starburst at the breakneck pace of 540 solar masses per year.
Galaxies of this era are “messier” than the ones we see in the nearby universe, the researchers say. Their more jumbled shapes would be due to the vast stores of gas raining down on them and their ongoing interactions and mergers with their neighbors.
Dark matter halo
The new observations also allowed the researchers to infer the presence of a truly massive dark matter halo surrounding both galaxies. Dark matter provides the pull of gravity that causes the universe to collapse into structures (galaxies, groups and clusters of galaxies, etc.).
“If you want to see if a galaxy makes sense in our current understanding of cosmology, you want to look at the dark matter halo—the collapsed dark matter structure—in which it resides,” says Chris Hayward, associate research scientist at the Center for Computational Astrophysics at the Flatiron Institute in New York City. “Fortunately, we know very well the ratio between dark matter and normal matter in the universe, so we can estimate what the dark matter halo mass must be.”
By comparing their calculations with current cosmological predictions, researchers found that this halo is one of the most massive that should exist at that time.
“There are more galaxies discovered with the South Pole Telescope that we’re following up on,” says Joaquin Vieira of the University of Illinois, Urbana-Champaign, “and there is a lot more survey data that we are just starting to analyze. Our hope is to find more objects like this, possibly even more distant ones, to better understand this population of extreme dusty galaxies and especially their relation to the bulk population of galaxies at this epoch.”
“In any case, our next round of ALMA observations should help us understand how quickly these galaxies came together and improve our understanding of massive galaxy formation during reionization,” Marrone says.
Source: University of Arizona
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