The Ejection and Detectability of High- and Hypervelocity Stars by Compact Object Binaries in Globular Clusters

The dense cores of Milky Way globular clusters (GCs) play host to a variety of dynamical encounters between stellar objects, which can accelerate stars to velocities high enough to escape the GC. The most extreme examples of these encounters are interactions between single GC stars and binaries including at least one compact object. These interactions can result in ejection velocities of up to several hundred km s −1 , approaching or exceeding the escape velocity of the Galaxy itself. In order to study whether these interactions contribute to the Galactic population of hypervelocity stars (stars moving faster than the Galactic escape speed), we combine Monte Carlo N -body GC simulations, observations of Galactic GCs, and a particle spray code to generate realistic populations of stars that have escaped from Milky Way GCs following star + compact object binary (S+COB) interactions. We find that over the last 500 Myr, S+COB interactions have likely ejected ∼6300 stars from Galactic GCs, of which 83 9 − 67 + 70 have present-day velocities exceeding 500 km s −1 . Using mock photometric observations, we find that 29 0 − 23 + 28 ejected stars are detectable in Gaia Data Release 3; however, only 1 − 1 + 2 stars faster than 500 km s −1 are detectable. Even so, we show that observational prospects in the upcoming Legacy Survey of Space and Time are more optimistic, and future detected fast extratidal GC stars will serve as a useful probe of GC cores.