Astronomers confirm collision of Milky Way satellite galaxies

Direct evidence of contact between the Large and Small Magellanic Clouds was provided by Gaia telescope

Photo: NASA The Small Cloud of Magellan, containing several hundred million stars

If you're standing in the Southern Hemisphere on a clear night, you can see two luminous clouds offset from the Milky Way. These clouds of stars are actually satellite galaxies of the Milky Way, called the Small Magellanic Cloud and the Large Magellanic Cloud, or SMC and LMC, respectively. Using the newly released data from a new, powerful space telescope, US astronomers have discovered that the southeast region, or "Wing," of the Small Magellanic Cloud is moving away from the main body of that dwarf galaxy, providing the first unambiguous evidence that the Small and Large Magellanic Clouds collided as recently as a few hundred million years ago.

"This is really one of our exciting results," said U-M professor of astronomy Sally Oey, lead author of the study, which was published in The Astrophysical Journal Letters. "You can actually see that the Wing is its own separate region that's moving away from the rest of the SMC."

Together with an international team, Oey and undergraduate researcher Johnny Dorigo Jones were examining the SMC for "runaway" stars, or stars that have been ejected from. 

For their observation the US researchers were using a recent data release from Gaia, a new, orbiting telescope launched by the European Space Agency, designed to image stars again and again over a period of several years in order to plot their movement in real time. In one mechanism, called the binary supernova scenario, one star in a gravitationally bound, binary pair explodes as a supernova, ejecting the other star like a slingshot. This mechanism produces X-ray-emitting binary stars. Another mechanism is that a gravitationally unstable cluster of stars eventually ejects one or two stars from the group. This is called the dynamical ejection scenario, which produces normal binary stars. That way, scientists could measure stars' individual velocities across the sky. They found significant numbers of runaway stars among both X-ray binaries and normal binaries, indicating that both mechanisms are important in ejecting stars from clusters.

In looking at the data, the team also observed that all the stars within the Wing - that southeast part of the SMC - are moving in a similar direction and speed. This demonstrates the SMC and LMC likely had a collision a few hundred million years ago.

"It's really interesting that Gaia obtained the proper motions of these stars. These motions contain everything we're looking at," Dorigo Jones said.

Study contributor Gurtina Besla, an astronomer at the University of Arizona, modeled the collision of the SMC and LMC. She and her team predicted a few years ago that a direct collision would cause the SMC Wing region to move toward the LMC, whereas if the two galaxies simply passed near each other, the Wing stars would be moving in a perpendicular direction. Instead, the Wing is moving away from the SMC, toward the LMC, said Oey, confirming that a direct collision occurred.

"We want as much information about these stars as possible to better constrain these ejection mechanisms," Dorigo Jones said. "Everyone loves marveling at images of galaxies and nebulae that are incredibly far away. The SMC is so close to us, however, that we can see its beauty in the night sky with just our naked eye. This fact, along with the data from Gaia, allow us to analyze the complex motions of stars within the SMC and even determine factors of its evolution."

Similar articles