Cosmic Cold Gas Pipelines Detected Feeding Early, Massive Galaxies
Researchers led by the University of Iowa have produced direct observational evidence that massive galaxies in the early universe were fed by cold gas pipelines that survived despite hotter surroundings and allowed these galaxies to form stars.
Credit: Hai Fu, University of Iowa ENLARGE
To come into being, galaxies need a steady diet of cold gases to undergo gravitational collapse. The larger the galaxy, the more cold gas it needs to coalesce and to grow.
Massive galaxies found in the early universe needed a lot of cold gas — a store totaling as much as 100 billion times the mass of our sun.
But where did these early, super-sized galaxies get that much cold gas when they were hemmed in by hotter surroundings?
In a new study, astronomers led by the University of Iowa report direct, observational evidence of streams of cold gas they believe provisioned these early, massive galaxies. They detected cold gas pipelines that knifed through the hot atmosphere in the dark matter halo of an early massive galaxy, supplying the materials for the galaxy to form stars.
About two decades ago, physicists working with simulations theorized that during the early universe, cosmic filaments ferried cold gas and embryonic, node-shaped galaxies to a dark matter halo, where it all clumped together to form massive galaxies. The theory assumed the filaments would need to be narrow and densely filled with cold gas to avoid being peeled off by the hotter surrounding atmosphere.
But the theory lacked direct evidence. In this study, scientists studied a gaseous region surrounding a massive galaxy formed when the universe was about 2.5 billion years old, or just 20% of its present age. The galaxy was previously unstudied, and it took the team five years to pinpoint its exact location and distance (through its redshift). The team needed a specially equipped observatory, the Atacama Large Millimeter/Submillimeter Array, because the target galaxy’s environment is so dusty that it can only be seen in the submillimeter range of the electromagnetic spectrum.
“It is the prototype, the first case where we detected a halo-scale stream that is feeding a very massive galaxy,” says Hai Fu, associate professor in Iowa’s Department of Physics and Astronomy and the study’s lead and corresponding author. “Based on our observations, such streams can fill up the reservoir in about a billion years, which is far shorter than the amount of time that was available to the galaxy at the epoch that we were observing.”