MiMeS项目：概述和现状
The MiMeS Project: Overview and Current Status
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950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。这种光谱和磁性材料的质量非常高，协作组渴望与能够以新的或不可预见的方式利用数据的同事建立联系。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状况。
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 950 high-resolution polarised spectra of about 150 individual stars with spectral types from B5-O4, discovering new magnetic fields in a dozen hot, massive stars. The quality of this spectral and magnetic matériel is very high, and the Collaboration is keen to connect with colleagues capable of exploiting the data in new or unforeseen ways. 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.
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。
