University of Texas at Austin astronomers studied 166 of the most massive galaxies present only a few billion years after the Big Bang.
Artist's concept of a disky galaxy growing rapidly via narrow streams of cold gas. The gas provided by these filaments likely fuels the prodigious star formation activity detected in many of these young, disky, massive galaxies. This process, called 'cold-mode accretion,' has never been directly observed, but Weinzirl and Jogee's findings of a large percentage of massive, disky star-forming galaxies 10 billion years ago suggests that it played an important role in those galaxies' formation. (ESA-AOES Medialab)
AUSTIN, Texas — A Hubble Space Telescope study of massive galaxies two to three billion years after the Big Bang has uncovered two remarkable results that challenge the common lore that major mergers play a dominant role in growing galaxies over a wide range of cosmic epochs.
Tim Weinzirl and Shardha Jogee, both from the University of Texas at Austin, studied 166 of the most massive galaxies present only a few billion years after the Big Bang, selected from the GOODS NICMOS survey headed by Christopher Conselice from the University of Nottingham in the United Kingdom.
“This is one of the largest near-infrared surveys of massive galaxies in the early universe conducted with the Hubble Space Telescope,” Conselice said.
The 166 selected galaxies contain between 50 billion to half a trillion solar masses worth of stars. Even at such early epochs, many of these young massive galaxies already harbor more stars than our Milky Way, a spiral galaxy containing about 80 billion stars.
Weinzirl led an extensive, sophisticated analysis that found that 60 percent of these massive young galaxies present two to three billion years after the Big Bang have a disk component, making them look like a thick pancake.
In contrast, today’s most massive galaxies — their descendants — typically have large bulges. They are shaped like watermelons, and are called elliptical galaxies, which contain just a bulge, and lenticular galaxies, which have both a bulge and a disk.
“These massive galaxies of the past are five times more likely to be disk-shaped than their descendants,” Weinzirl said.
Another difference is that “many of these disky massive galaxies are prodigious star factories,” Jogee said. “They are churning new young stars over 100 times faster than present-day massive galaxies.”
Finding such a large fraction of massive galaxies with disk-like properties two to three billion years after the Big Bang has far-reaching implications. “It challenges models of galaxy growth, particularly the popular idea that galaxies grow in mass primarily via the violent major merger of galaxies,” Jogee said.
A “major merger” is the violent merger of two galaxies of similar mass, and it can radically transform two merging spiral galaxies into a new system that is no longer a disk-dominated galaxy, but instead has a prominent bulge. If major mergers dominated galaxy growth at early cosmic epochs, one would expect to find most galaxies to be dominated by bulges rather than by disks.
“Even considering the latest theoretical simulations of more extreme, very gas-rich major mergers does not solve the problem,” Weinzirl said. Instead, the results suggest that another process, called “cold mode accretion” plays a key role in growing massive galaxies at early cosmic epochs. In that process, galaxies grow in mass by accreting cold gas from large-scale cosmological filaments.
Weinzirl and Jogee’s study raises a second baffling challenge. Just like toddlers growing up, these massive young galaxies are expected to increase their mass over time. They have to turn into the most massive galaxies present in today’s universe, the elliptical and lenticular galaxies. This transformation is nothing short of dramatic, as the progenitors and descendants are radically different in size, shape, and structure.
Their study showed that as many as 40 percent of the young massive galaxies are ultra-compact — half of their light and mass are jam-packed into a small amount of space (less than 65,000 light-years in radius), Weinzirl said. In contrast, less than 1 percent of their descendants, today’s massive elliptical and lenticular galaxies, are ultra-compact. Most are much larger and more spread out.
Furthermore, while many of the massive young galaxies are disky galaxies — shaped like thick pancakes — massive ellipticals and lenticulars tend to be dominated by bulges — shaped like watermelons.
“While major mergers can morph some disky galaxies into bulgy ones, and produce part of observed growth in size, there simply does not seem to be enough major mergers to produce the full blow-up in size needed,” Jogee said.
Instead, some of the latest theoretical simulations suggest that minor mergers — in which a large galaxy swallows a smaller galaxy — might hold the key.
“Minor mergers are much more common than major ones because there are more lower-mass galaxies than there are very massive galaxies,” Weinzirl said, and they “likely drive the growth of ultra-compact galaxies into more extended galaxies.”
“The bottom line is that our study, and a rising body of evidence from other lines of inquiry, now suggest that violent major mergers have been overrated. They are spectacular cosmic fireworks, but they do not necessarily drive galaxy growth at all epochs,” Jogee said.
There’s plenty more work to be done in understanding the evolution of massive galaxies. On the theoretical front, “simulations have yet to reproduce the widely diverse massive young galaxies, running the gamut from ultra-compact to extended disky systems, and from quiescent to widely star-forming,” Weinzirl said.
On the observational frontier, “we are thrilled that the next generation 25-meter Giant Magellan Telescope will provide unparalleled insights into massive young galaxies and the physics of major mergers at early cosmic epochs,” Jogee said.
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