论文标题
使用Polstar的紫外线光谱法:使用polstar测试磁层质量减震
Ultraviolet Spectropolarimetry With Polstar: Using Polstar to test Magnetospheric Mass-loss Quenching
论文作者
论文摘要
POLSTAR是提出的NASA Midex空间望远镜,将在远紫外线中提供高分辨率的同时全孔光谱法,并在近紫外线中以及低分辨率的线性极化法。该天文台提供了前所未有的功能,可以获取有关热星磁层的磁性和等离子体特性的独特信息。我们描述了一种观察程序,利用已知的磁热星人群来测试磁层应作用以迅速排出角动量的基本假设,从而使恒星向下旋转,同时降低净质量损失率。这两种作用都预计会导致磁性与非磁星的演变的巨大差异。
Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far ultraviolet, together with low-resolution linear polarimetry in the near ultraviolet. This observatory offers unprecedented capabilities to obtain unique information on the magnetic and plasma properties of the magnetospheres of hot stars. We describe an observing program making use of the known population of magnetic hot stars to test the fundamental hypothesis that magnetospheres should act to rapidly drain angular momentum, thereby spinning the star down, whilst simultaneously reducing the net mass-loss rate. Both effects are expected to lead to dramatic differences in the evolution of magnetic vs. non-magnetic stars.