Washington: A team of researchers have found a way to reconstruct the evolutionary history of our galaxy, the Milky Way, to a new level of detail.
For this study, Ivan Minchev from the Leibniz Institute for Astrophysics Potsdam (AIP) and his team took advantage of high-quality data regarding stars close to the Sun from the RAdial Velocity Experiment (RAVE). The scientists found that the rule of thumb "the older a star is, the faster it moves up and down through the disc" did not apply to the stars with the highest magnesium-to-iron ratios.
Contrary to expectations, scientists observed an extreme drop in the vertical speed for these stars.
To understand these surprising observations, the scientists ran a computer model of the Milky Way, which allowed them to examine the origin of these slow-moving, old stars.
After studying the computer model, they found that small galactic collisions might be responsible. It is thought that the Milky Way has undergone hundreds of such collisions with smaller galaxies in the course of its history.
These collisions are not very effective at shaking up the massive regions near the galactic center. However they can trigger the formation of spiral arms and as a consequence move stars from the center of the galaxy to the outer parts, where the Sun is.
This "radial migration" process is able to transport outward old stars (with high values of magnesium-to-iron ratio) and with low up-and-down velocities. Therefore, the best explanation for why the oldest stars near our Sun have such small vertical velocities is that they were forced out of the galactic center by galactic collisions.
The difference in speed between those stars and the ones born close to the Sun thereby betray how massive and how numerous the merging satellite galaxies were.