  Exoplanets display incredible diversity, from planetary system architectures
around Sun-like stars that are very different to our Solar System, to planets
orbiting post-main sequence stars or stellar remnants. Recently the B-star
Exoplanet Abundance STudy (BEAST) reported the discovery of at least two
super-Jovian planets orbiting massive stars in the Sco Cen OB association.
Whilst such massive stars do have Keplerian discs, it is hard to envisage gas
giant planets being able to form in such hostile environments. We use N-body
simulations of star-forming regions to show that these systems can instead form
from the capture of a free-floating planet, or the direct theft of a planet
from one star to another, more massive star. We find that this occurs on
average once in the first 10Myr of an association's evolution, and that the
semimajor axes of the hitherto confirmed BEAST planets (290 and 556au) are more
consistent with capture than theft. Our results lend further credence to the
notion that planets on more distant (>100au) orbits may not be orbiting their
parent star.
