In a paper published in the journal Monthly Notices of the Royal Astronomical Society, the researchers explain that they wanted to discover why high-speed stars have mainly been recorded in the Northern Hemisphere. If the supermassive black hole theory was correct, the stars would be more evenly-distributed across the sky.
The alternative explanation? The stars are runaways from a binary system. In binary star systems, the closer the two stars are, the faster they orbit one another. If one star explodes as a supernova, it can break up the binary and the remaining star flies off at the speed it was orbiting. The escaping star is known as a runaway.
The LMC is the perfect environment for this, according to the researchers. It's the largest and fastest of the dozens of dwarf galaxies in orbit around the Milky Way -- careening it at around 400 kilometers per second. It only has 10 percent of the mass of the Milky Way, so the fastest runaways born in this dwarf galaxy can easily escape its gravity.
"These stars have just jumped from an express train -- no wonder they're fast," said co-author Rob Izzard, a Rutherford fellow at the Institute of Astronomy. "This also explains their position in the sky, because the fastest runaways are ejected along the orbit of the LMC towards the constellations of Leo and Sextans."
The team is the first to simulate the ejection of runaway stars from the LRC, and will know as soon as next year whether its theory is correct.
"We'll know soon enough whether we're right," said co-author Douglas Boubert. "The European Space Agency's Gaia satellite will report data on billions of stars next year, and there should be a trail of hypervelocity stars across the sky between the Leo and Sextans constellations in the north and the LMC in the South."