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Alejandro Benitez-Llambay
A visualization of cosmic web stripping, which bleeds away matter from the fastest-moving dwarf galaxies in the Local Group.
By Elizabeth Howell
Space.com
Some dwarf galaxies in the early universe traveled so fast that their gas was stripped from them, according to a new computer simulation.
This cosmic vanishing act could help explain a long-standing mystery: astronomers observe fewer dwarf galaxies in the "Local Group" — the collection of galaxies near the Milky Way — than what models of the universe's formation predict.
But if these galaxies are losing gas, that could explain why they don't appear as plentiful as they should.
Because these dwarf galaxies were so small when they formed, they don't have large reserves of gas to begin with. Stripping any gas away would leave these galaxies so small and dim that they would be all but invisible from Earth. [Stunning Photos of Our Milky Way Galaxy]
"This is something that came out of the simulations, and had not been anticipated, and had not been seen before. It was an interesting discovery," said Julio Navarro, a University of Victoria astronomer and co-author of a paper describing the discovery.
The study, published in the Feb. 1 issue of Astrophysical Journal Letters,was led by graduate student Alejandro Benitez-Llambay from the University of Cordoba in Argentina. You can also watch a Space.com video explaining the missing dwarf galaxies.
Courting CLUES
Past supercomputer simulations show there should be a huge number of dwarf galaxies, together making up one one-thousandth of the Milky Way's mass, scattered around the local environment. But a 1999 study pointed out that the dwarf galaxies we see are not representative of the calculated mass.
In the past, astronomers suggested that the energy from supernovas, as well as ultraviolet rays permeating the universe, might alter the dwarf galaxies as they form. There were weaknesses with these models, however. Observed supernova energy is too low to affect dwarf galaxy formation, and the ultraviolet rays only shrink the smallest of dwarf galaxies.
To better examine the issue, the new study focused on how dwarf galaxies evolved in the early stages of the universe. Astronomers ran a simulation tracking dark matter halos that duplicate the positions of the three largest galaxies in the Local Group: the Milky Way, Andromeda (M31) and Triangulum (M33).
Next, they re-ran the simulation to focus on one small area in much higher resolution. This allowed them to examine dwarf galaxy evolution in detail.
"We constrained and controlled the numbers to resemble our local environment," Navarro said.
The tool they used was called Constrained Local UniversE Simulations, or CLUES for short. The project, led by the Leibniz Institute for Astrophysics, can simulate the positions and speeds of galaxies within 10 million light years of the Milky Way.
Passing the cosmic speed limit
CLUES revealed that the farthest dwarf galaxies in the Local Group are flying very quickly through the cosmic web of dark matter and ordinary matter that make up our universe.
When the galaxies pass a given speed, the ram pressure between the dwarf galaxies and this cosmic web strips the galaxies' gas away. It's similar to how the matter gets stripped away from a meteor as it rams through the Earth's atmosphere.
"The galaxy moves at high speed, and the gas strips out and stays behind the galaxy," said Stefan Gottlöber, a Leibniz astronomer who leads CLUES. He was also a co-author on the new paper.
While the gas is all but invisible, we might be able to see the effects gas stripping has had on the galaxies. The astronomers noted that dwarf galaxies are a diverse bunch, with some looking like gas clouds and others filled with stars. Gas stripping could explain why star formation stopped, the scientists suggested.
Navarro, Gottloeber and their collaborators plan another run with CLUES to simulate a larger area to test whether the dwarf galaxy stripping in the Local Group is representative of the entire universe.
Follow Elizabeth Howell @howellspace, or Space.com @Spacedotcom. We're also on Facebook and Google+. Original article on Space.com.
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Leave a Comment:
I'd rather we spend the time on finding all of that vanishing taxes we paid that uncle Sam uses for it's own wants and desires.
You mean the wants and desires of the representatives that you democratically elect.
The technology doesn't exist.
I think finding your vanishing brain cells is far higher priority.
I don't quite understand how this works. The gas rams dark matter? Doesn't this model then depend on ordinary matter and dark matter interacting?
Yes, it would interact gravitationally, but all matter would be affected, including that in the stars themselves, so the dwarf galaxy's stars and gas should move as a unit.
And where would the ordinary matter being rammed come from? Isn't all of it already in the dwarf galaxy?
I am sure all these questions are easily explained, but I can't figure them out from reading the article. What does the cosmic web consist of?
I have a related question that I hope someone could shed some light on:
I understand that the Milky Way Galaxy is (or was) being intersected by a dwarf galaxy. I believe that this dwarf galaxy was given the name, Sagittarius.
Others speculated that our solar system could really be a member of that galaxy instead of the Milky Way. It was based upon the belief that the trajectory of our system in relation to the other star systems that revolve around the Milky Way's center was different and followed Sagittarius Dwarf's trajectory.
Does anyone know anything about our trajectory as it relates to the Milky Way's ecliptic plane?
Is it traveling parallel to this plane or at an angle?
Hiya RFBS!
There some two dozen dwarf galaxies so far identified that are in the process of being absorbed into the Milky Way Galaxy; the Sagittarius dwarf is one of those.
(There are also some 150 or so globular star clusters so far found orbiting the Milky Way; many, or perhaps most, of those are the remnants of past dwarf galaxies that have been subsumed into the MW.)
Our Sun's orbit around the Milky Way is entirely consistent with the Sun being created IN the Milky Way, and not a captured dwarf galaxy object. Our orbit is indeed pretty much parallel to the galactic disk, orbiting in the same general direction and speed as the other stars in the Orion Arm that are our neighbours.
It took us a while to be fairly certain, but yes; we are home-grown here in the Milky Way.
Cheers! ~Michael (Astronomy.FM★Radio)
Michael,
Thank you for this information.
And, thanks for your educated and polite reply.
I think it would be far better to solve the mystery of vanishing government funds which amount to the tens of billions a year--if not hundreds of billions.
Do you know how many drones it takes to strip the gas away from a dwarf galaxy?