论文标题
近红外和视觉高分辨率偏振成像与AO系统
Near-IR and visual high resolution polarimetric imaging with AO systems
论文作者
论文摘要
近年来，通过大型望远镜的自适应光学器械（AO）仪器获得了许多壮观的极化图像，因为它们从高空间分辨率中获得了显着的利润。本文总结了AO极化法的一些基本原理，讨论了这些系统的挑战和局限性，并描述了结果，这些结果说明了AO极化器的性能，用于研究Interellar磁盘，进化的星星的尘土飞扬的风以及搜索反射额外星球的尘土飞扬。
Many spectacular polarimetric images have been obtained in recent years with adaptive optics (AO) instruments at large telescopes because they profit significantly from the high spatial resolution. This paper summarizes some basic principles for AO polarimetry, discusses challenges and limitations of these systems, and describes results which illustrate the performance of AO polarimeters for the investigation of circumstellar disks, of dusty winds from evolved stars, and for the search of reflecting extra-solar planets.
