“Unknown Phenomenon” –36 Distant Dwarf Galaxies had Simultaneous Creation of New Stars

36 Dwarf Galaxies


An unknown phenomenon has been discovered in the Universe: three dozen dwarf galaxies far from each other had a simultaneous birth of new stars, an unexpected discovery that challenges current theories on how galaxies grow and may enhance our understanding of the universe.

Unknown Extra-galactic Social Network

Galaxies more than 1 million light-years apart should have completely independent lives in terms of when they give birth to new stars. But galaxies separated by up to 13 million light-years slowed down and then simultaneously accelerated their birth rate of stars, according to a Rutgers-led study published in the Astrophysical Journal.

“It appears that these galaxies are responding to a large-scale change in their environment in the same way a good economy can spur a baby boom,” said lead author Charlotte Olsen, a doctoral candidate in the Department of Physics and Astronomy at Rutgers University

“We found that regardless of whether these galaxies were next-door neighbors or not, they stopped and then started forming new stars at the same time, as if they’d all influenced each other through some extra-galactic social network,” said co-author Eric Gawiser, a professor in the Department of Physics and Astronomy.

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Connected by a Large Cosmic Filament?

“A large cosmic filament could be an option, but we don’t yet know enough about this phenomena to infer its cause,” said Olsen in reply to an email from The Daily Galaxy. “Before speculating about whether a large-scale environmental effect could be responsible for this finding, we want to get a better handle on its extent. We need to look more deeply into the Local Volume and beyond to see if this is relatively local, or if this was happening all over the universe at the same time. Once we know that, we might be able to start drawing conclusions, or at least ruling things out.” 

The simultaneous decrease in the stellar birth rate in the 36 dwarf galaxies began 6 billion years ago, and the increase began 3 billion years ago. Understanding how galaxies evolve requires untangling the many processes that affect them over their lifetimes (billions of years). Star formation is one of the most fundamental processes. The stellar birth rate can increase when galaxies collide or interact, and galaxies can stop making new stars if the gas (mostly hydrogen) that makes stars is lost.

Star formation histories can paint a rich record of environmental conditions as a galaxy “grew up.” Dwarf galaxies are the most common but least massive type of galaxies in the universe, and they are especially sensitive to the effects of their surrounding environment.

A Phenomenon in the Universe We Don’t Yet Know About

The 36 dwarf galaxies included a diverse array of environments at distances as far as 13 million light-years from the Milky Way. The environmental change the galaxies apparently responded to must be something that distributes fuel for galaxies very far apart. That could mean encountering a huge cloud of gas, for example, or a phenomenon in the universe we don’t yet know about, according to Olsen.

The scientists used two methods to compare star formation histories. One uses light from individual stars within galaxies; the other uses the light of a whole galaxy, including a broad range of colors.

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 Full Impact of the Discovery Not Yet Known

“The full impact of the discovery is not yet known as it remains to be seen how much our current models of galaxy growth need to be modified to understand this surprise,” Gawiser said. “If the result cannot be explained within our current understanding of cosmology, that would be a huge implication, but we have to give the theorists a chance to read our paper and respond with their own research advances.”

“The James Webb Space Telescope, scheduled to be launched by NASA this October, will be the ideal way to add that new data to find out just how far outwards from the Milky Way this ‘baby boom’ extended,” Olsen added.

Maxwell Moe, astrophysicist, NASA Einstein Fellow, University of Arizona via Rutgers University and Charlotte Olsen



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