"This is different from what we see in the nearby Universe, where galaxies in clusters grow by cannibalising other galaxies," said Bjorn Emonts of the Centre for Astrobiology in Spain, who led the study.
"In this cluster, a giant galaxy is growing by feeding on the soup of cold gas in which it is submerged," said Emonts.
The scientists studied an object called the Spiderweb Galaxy, which actually is not yet a single galaxy, but a clustering of protogalaxies more than 10 billion light-years from Earth.
The astronomers used the Australia Telescope Compact Array (ATCA) and the National Science Foundation's Very Large Array (VLA) to detect carbon monoxide (CO) gas.
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The presence of the CO gas indicates a larger quantity of molecular hydrogen, which is much more difficult to detect.
The astronomers estimated that the molecular gas totals more than 100 billion times the mass of the Sun.
Not only is this quantity of gas surprising, they said, but the gas also must be unexpectedly cold, about minus-200 degrees Celsius. Such cold molecular gas is the raw material for new stars.
The carbon and oxygen in the CO was formed in the cores of stars that later exploded.
The ATCA observations revealed the total extent of the gas, and the VLA observations, much more narrowly focused, provided another surprise. Most of the cold gas was found, not within the protogalaxies, but instead between them.
"This is a huge system, with this molecular gas spanning three times the size of our own Milky Way Galaxy," said Preshanth Jagannathan, of the US National Radio Astronomy Observatory (NRAO).
"It appears that this whole system eventually will collapse into a single, gigantic galaxy," Jagannathan said.
"These observations give us a fascinating look at what we believe is an early stage in the growth of massive galaxies in clusters, a stage far different from galaxy growth in the current Universe," said Chris Carilli of NRAO.
The study was published in the journal Science.