The Nature of Hypervelocity Stars and the Time Between Their Formation and Ejection

TL;DR

This study analyzes hypervelocity star HVS5, revealing an unexpected delay between its formation and ejection, supporting a Galactic center origin and providing insights into star ejection timescales and Galactic center star formation history.

Contribution

It presents the first detailed age and ejection time analysis of HVS5, challenging existing ejection models and supporting a Galactic center origin for hypervelocity stars.

Findings

HVS5 is a 3.62 Msun main sequence star at 50 kpc.

The delay between formation and ejection is about 105 Myr.

Ejection during the first 10 Myr of its life is ruled out.

Abstract

We obtain Keck HIRES spectroscopy of HVS5, one of the fastest unbound stars in the Milky Way halo. We show that HVS5 is a 3.62 +- 0.11 Msun main sequence B star at a distance of 50 +- 5 kpc. The difference between its age and its flight time from the Galactic center is 105 +-18(stat)+-30(sys) Myr; flight times from locations elsewhere in the Galactic disk are similar. This 10^8 yr `arrival time' between formation and ejection is difficult to reconcile with any ejection scenario involving massive stars that live for only 10^7 yr. For comparison, we derive arrival times of 10^7 yr for two unbound runaway B stars, consistent with their disk origin where ejection results from a supernova in a binary system or dynamical interactions between massive stars in a dense star cluster. For HVS5, ejection during the first 10^7 yr of its lifetime is ruled out at the 3-sigma level. Together with the 10^8 yr arrival times inferred for three other well-studied hypervelocity stars (HVSs), these results are consistent with a Galactic center origin for the HVSs. If the HVSs were indeed ejected by the central black hole, then the Galactic center was forming stars ~200 Myr ago, and the progenitors of the HVSs took ~100 Myr to enter the black hole's loss cone.