Stoop, MitchelKoter, Alex deKaper, LexBrands, SarahPortegies Zwart, SimonSana, HuguesStoppa, FiorenzoGieles, MarkMahy, LaurentShenar ,TomerGuo, DifengNelemans, GijsRieder, Steven2025-07-102025-07-102024-10-240028-0836https://hdl.handle.net/2445/222131Massive stars are predominantly born in stellar associations or clusters [1]. The irradiation fields, stellar winds, and supernovae strongly impact their local environment. In the first few million years of a cluster’s life, massive stars are dynamically1arXiv:2410.06255v1 [astro-ph.SR] 8 Oct 2024 rejected running away from the cluster at high speed [2]. However, the production rate of dynamically ejected runaways is poorly constrained. Here we report on a sample of 55 massive runaway stars ejected from the young cluster R136in the Large Magellanic Cloud. Astrometric analysis with Gaia [3–5] reveals two channels of dynamically ejected runaways. The first channel ejects massive stars in all directions and is consistent with dynamical interactions during and after the birth of R136. The second channel launches stars in a preferred direction and may be related to a cluster interaction. We find that 23-33% of the most luminous stars initially born in R136 are runaways. Model predictions [2, 6, 7] have significantly underestimated the dynamical escape fraction of massive stars. Consequently, their role in shaping and heating the interstellar and galactic medium,along with their role in driving galactic outflows, is far more important than previously thought.39 p.application/pdfeng(c) Nature Publishing Group, 2024Formació d'estelsDinàmica estel·larCúmuls d'estelsStar formationStellar dynamicsClusters of starsinfo:eu-repo/semantics/article7570062025-07-10info:eu-repo/semantics/openAccess