Science with Adaptive Optics
Science with Adaptive Optics
复制标题
自适应光学科学
DOI：
10.1007/b80350
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发表时间：
2005
期刊：
影响因子：
--
通讯作者：
M. Kasper
中科院分区：
文献类型：
--
作者：
W. Brandner;M. Kasper
近年来，天文学的自适应光学（AO）领域已经成熟，近红外线的衍射极限图像分辨率现在通常由地面8至10米级望远镜实现。这本书介绍了在2003年秋季举行的ESO自适应光学科学研讨会的会议记录。这本书提供了AO仪器，数据采集和减少策略的概述，并涵盖了太阳，太阳系天体，拱星盘，亚恒星同伴，HII地区，星暴环境，晚型恒星，银河系中心，活动星系和类星体的观测。这些贡献生动地描绘了AO在观测天文学中所处理的众多科学主题。
The field of Adaptive Optics (AO) for astronomy has matured in recent years, and diffraction-limited image resolution in the near-infrared is now routinely achieved by ground-based 8 to 10m class telescopes. This book presents the proceedings of the ESO Workshop on Science with Adaptive Optics held in the fall of 2003. The book provides an overview on AO instrumentation, data acquisition and reduction strategies, and covers observations of the sun, solar system objects, circumstellar disks, substellar companions, HII regions, starburst environments, late-type stars, the galactic center, active galaxies, and quasars. The contributions present a vivid picture of the multitude of science topics being addressed by AO in observational astronomy.