The runaway nature and origin of {\alpha} Crucis system

TL;DR

This study investigates the { extalpha} Crucis system's motion and bow shock, concluding it is not a runaway star but moves with its stellar cluster, based on Gaia and WISE data analysis.

Contribution

The paper provides new insights into the origin and motion of the { extalpha} Crucis system, demonstrating it is part of a stellar cluster and not a runaway star.

Findings

{ extalpha} Crucis moves with its cluster at ~1.3 km/s.

The bow shock is consistent with interstellar medium motions.

The system is not a runaway star, contrary to previous assumptions.

Abstract

Massive stars are always the focus of astronomical research and a significant part of them (10--20%) moves in space at a high (supersonic) velocity. This paper presents the results of a study of the $\alpha$ Crucis system, located at $\sim$114 pc distance from the Sun, with an observed bow shock around it. We used data and images from the Gaia and WISE space telescopes. The coordinates, distance, and proper motion of the $\alpha$ Crucis system were used to determine its space velocity. We managed to find a stellar cluster to which the $\alpha$ Crucis system belongs, that is, it has not been ejected from its parent cluster, but is moving in space together with other members of the cluster. The $\alpha$ Crucis system has a velocity of $\sim$1.3 km/s relative to the star cluster. The geometric parameters of the bow shock are compatible with other known bow shocks. The bow shock is unaligned, i.e., most likely interstellar medium large-scale motions are responsible for the resulting bow shock, which is further evidence that the $\alpha$ Crucis system is not runaway in nature.