MiMeS项目：现状和最新成果
The MiMeS Project: Current status and recent results
摘要：
大质量恒星中的磁性（MiMeS）项目是国际上许多最重要的热、大质量恒星物理学研究人员的共识合作，其基本目的是了解这些物体中磁场的起源、演变和影响。在撰写本文时，MiMeS大型计划已经获得了大约150颗恒星的1250多个高分辨率极化光谱，光谱类型来自B5-O 4，在十几颗热的大质量恒星中发现了新的磁场。值得注意的结果包括在两个最快速旋转的已知磁星和最大质量的已知磁星中检测到磁场。在本文中，我们回顾了结构的MiMeS观测计划和报告的观测，数据建模和相关理论的发展，并回顾迄今为止取得的重要成果。
英文摘要：
The Magnetism in Massive Stars (MiMeS) Project is a consensus collaboration among many of the foremost international researchers of the physics of hot, massive stars, with the basic aim of understanding the origin, evolution and impact of magnetic fields in these objects. At the time of writing, MiMeS Large Programs have acquired over 1250 high-resolution polarised spectra of about 150 individual stars with spectral types from B5-O4, discovering new magnetic fields in over a dozen hot, massive stars. Notable results include the detection of magnetic fields in the two most rapidly-rotating known magnetic stars, and in the most massive known magnetic star. In this paper we review the structure of the MiMeS observing programs and report the status of observations, data modeling and development of related theory, and review important results obtained so far.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
