Two waves of massive stars running away from the young cluster R136

• 成果类型: Article
• 署名作者: Stoop, Mitchel; de Koter, Alex; Kaper, Lex; Brands, Sarah; Portegies Zwart, Simon; Sana, Hugues; Stoppa, Fiorenzo; Gieles, Mark; Mahy, Laurent; Shenar, Tomer; Guo, Difeng; Nelemans, Gijs; Rieder, Steven
• 署名单位: University of Amsterdam; Leiden University; Leiden University - Excl LUMC; Radboud University Nijmegen; ICREA; Institut d'Estudis Espacials de Catalunya (IEEC); University of Barcelona; Tel Aviv University
• 刊物名称: Nature
• ISSN/ISSBN: 0028-4241
• DOI: 10.1038/s41586-024-08013-8
• 发表日期: 2024-10-01
• 页码: 809-+
• 关键词: large-magellanic-cloud; runaway star; origin; ultraviolet; galaxies

摘要

Massive stars are predominantly born in stellar associations or clusters(1). Their radiation fields, stellar winds and supernovae strongly impact their local environment. In the first few million years of a cluster's life, massive stars are dynamically ejected and run 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 R136 in the Large Magellanic Cloud. An astrometric analysis of Gaia data(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 found 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 media and their role in driving galactic outflows are far more important than previously thought(8,9).