论文标题
复杂的上HR图
The Complex Upper HR Diagram
论文作者
论文摘要
几十年来对最大和最发光的恒星的观察结果揭示了一个复杂的上HR图，其质量损失形状，并由各种进化的恒星居住，表现出其质量损失史的后果。这篇综述介绍了大型恒星的人力资源图的简要概述，突出了一些主要发现以及它们在附近星系中观察到的结果。本卷中的章节包括我们当前对不同群体巨大恒星的理解，所有这些都失去了质量和进化的不同阶段。发光的蓝色变量（LBV），b [e]超级巨人，温暖的超级巨人，狼射线星以及麦哲伦云中的OB恒星和超级巨星的种群。
Several decades of observations of the most massive and most luminous stars have revealed a complex upper HR Diagram, shaped by mass loss, and inhabited by a variety of evolved stars exhibiting the consequences of their mass loss histories. This review presents a brief historical overview of the HR Diagram for massive stars, highlighting some of the primary discoveries and results from their observation in nearby galaxies. The chapters in this volume include reviews of our current understanding of different groups of evolved massive stars, all losing mass and in different stages of their evolution; the Luminous Blue Variables (LBVs), B[e] supergiants, the warm hypergiants, Wolf-Rayet stars, and the population of OB stars and supergiants in the Magellanic Clouds.
