Colossal hydrogen bridge between galaxies could be fuel line for new stars
Researchers studying a filament of hydrogen between the Andromeda and Triangulum galaxies found rotating clumps of gas the size of dwarf galaxies. But questions remain.
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The new observations were made with a 100-meter-wide dish at the National Radio Astronomy Observatory's Greenbank facility in West Virginia. Although it's significantly more sensitive than the radio telescopes used previously, the team still had to push it to its limits.Skip to next paragraph
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“We were reaching sensitivities that have never been reached before,” says Edward Shaya, an astrophysicist at the University of Maryland at College Park, and a member of the team reporting its results in Thursday's issue of the journal Nature.
Within the neutral hydrogen dispersed in the larger stream of ionized hydrogen, the team found seven blobs that range in size from about 7,800 light-years across to 20,900 light-years across and contain gas supplies that could form between 40,000 and 400,000 suns.
Some researchers had suggested that the bridge really was a tail of material pulled from Andromeda by a close encounter with the Triangulum Galaxy.
But the team notes that the close encounter is thought to have taken place a few billion years ago. The lifetime of gas clumps on the scale the team detected would have collapsed to begin making stars some 400 million years after they formed. And given the length of the bridge, it would take only about 100 million years for a blob to cross it. Instead, the team suspects that the blobs formed spontaneously from some instabilities within the gas bridge.
Such instabilities could result from the gravitational influence of a filament of dark matter – a form of matter that doesn't readily interact with other forms of matter except through its gravity. Such a filament would serve as the bridge's scaffolding. The influence of dark matter also would explain the clustering the seven clumps exhibit, the researchers posit.
Invoking filaments of ionized hydrogen as the ultimate reservoir for the stuff of new stars also helps explain the reduced productivity in today's universe, Braun adds.
"The rate of condensation of ionized to neutral matter has slowed down as a consequence of the accelerating expansion of the universe due to dark energy, which has made it increasingly difficult to capture the ionized filaments of gas," he writes.
Now that the team has identified neutral hydrogen in the bridge, "the question we haven't resolved yet is whether this is gas that's falling in or is being drawn out,” Dr. Shaya says.
Nor has the team analyzed the full length of the bridge yet.
“There could be a heck of a lot more gas out there than we are aware of,” he adds.
If such bridges and clumps are common, they could help explain why stars continue to form in galaxies that, if left to their own resources, should have run out of gas long ago. But trying to find out how common is a tough task. The bridge is extraordinarily faint, while the galaxies at each end are the closest large spirals in the Milky Way's neighborhood.
“We have no hope of observing at this level for all the other galaxies,” he says.
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