# The Great Escape: Discovery of a nearby 1700 km/s star ejected from the Milky Way by Sgr A*

## TL;DR

The paper reports the discovery of S5-HVS1, the fastest known hyper-velocity star ejected from the Galactic Centre, providing new insights into Galactic dynamics and the star's origin.

## Contribution

It presents the first confirmed hyper-velocity star from the Galactic Centre with detailed velocity and trajectory analysis, linking it to the Galactic Centre's formation and dynamics.

## Key findings

- S5-HVS1 has a 3D velocity of 1755 km/s.
- The star was ejected from the Galactic Centre about 4.8 million years ago.
- The star's properties constrain the Galaxy's geometry and kinematics.

## Abstract

We present the serendipitous discovery of the fastest Main Sequence hyper-velocity star (HVS) by the Southern Stellar Stream Spectroscopic Survey (S5). The star S5-HVS1 is a $\sim 2.35$ M$_\odot$ A-type star located at a distance of $\sim 9$ kpc from the Sun and has a heliocentric radial velocity of $1017\pm 2.7$ km/s without any signature of velocity variability. The current 3-D velocity of the star in the Galactic frame is $1755\pm50$ km/s. When integrated backwards in time, the orbit of the star points unambiguously to the Galactic Centre, implying that S5-HVS1 was kicked away from Sgr A* with a velocity of $\sim 1800$ km/s and travelled for $4.8$ Myr to its current location. This is so far the only HVS confidently associated with the Galactic Centre. S5-HVS1 is also the first hyper-velocity star to provide constraints on the geometry and kinematics of the Galaxy, such as the Solar motion $V_{y,\odot}= 246.1\pm 5.3$ km/s or position $R_0=8.12\pm 0.23$ kpc. The ejection trajectory and transit time of S5-HVS1 coincide with the orbital plane and age of the annular disk of young stars at the Galactic centre, and thus may be linked to its formation. With the S5-HVS1 ejection velocity being almost twice the velocity of other hyper-velocity stars previously associated with the Galactic Centre, we question whether they have been generated by the same mechanism or whether the ejection velocity distribution has been constant over time.