210 citations · 1.9k across the 45 of their papers we have counts for
Showing 2026Show all
2 papers · 1 filter
astro-ph.SR2026
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry
J. van den Eijnden, L. Kaper
Bow shocks are one the most commonly observed impact sites of massive star feedback. Their existence is often taken as evidence of the supersonic motion or even runaway nature of t…
astro-ph.SR2026
OB runaway stars originating in the Vel OB1 association
N. Azatyan, L. Kaper, A. Samsonyan +4
OB runaway stars are massive stars moving through interstellar space at high velocities (up to 200 km/s), produced by dynamical ejections in young massive clusters or supernova exp…