Brown discovered the first
hypervelocity star in 2005.
And because the LMC is orbiting the Milky Way at nearly 400 kilometers per second, a star ejected from it could be moving faster than the 500 kilometers per second that makes
it a hypervelocity star in the Milky Way.
Not exact matches
As the team report today
in Monthly Notices of the Royal Astronomical Society and at the U.K. National Astronomy Meeting
in Hull, most of the known
hypervelocity stars have trajectories that would fit this scenario.
But a new study shows that most of the 20 or so
hypervelocity stars found so far might actually come from outside our own galaxy,
in the Large Magellanic Cloud, a small satellite galaxy orbiting the Milky Way at nearly 400 kilometers per second.
In the case 2), the candidate is a
hypervelocity star which moves so fast that it can escape from the gravity of the Galaxy.
US 708 has another peculiar property
in marked contrast to other
hypervelocity stars: it is a rapidly rotating, compact helium
star likely formed by interaction with a close companion.
These astronomers were able to measure the relative abundances of certain elements for the first time
in any
hypervelocity star.
Discovered
in 2005, US 708 differs from other known
hypervelocity stars.
hypervelocity An adjective for
stars that move across space at unusual speed — enough speed,
in fact, that they can escape the gravitational hold of their parent galaxy.