Near-infrared polarimetry of the GG Tauri A binary system

A high angular resolution near-infrared image that shows the intensity of polarization for the GG Tau A binary system was obtained with the Subaru Telescope. The image shows a circumbinary disk scattering the light from the central binary. The azimuthal profile of the intensity of polarization for the circumbinary disk is roughly reproduced by a simple disk model with the Henyey-Greenstein phase function and the Rayleigh function, indicating there are small dust grains at the surface of the disk. Combined with a previous observation of the circumbinary disk, our image indicates that the gap structure in the circumbinary disk orbits counterclockwise, but material in the disk orbits clockwise. We propose that there is a shadow caused by material located between the central binary and the circumbinary disk. The separations and position angles of the stellar components of the binary in the past 20 yr are consistent with the binary orbit with a = 33.4 AU and e = 0.34.

基于自参考的高精度红外点衍射干涉仪研制(英文)

介绍了一种结构简单紧凑、可用于高精度实时相位波前测量的红外点衍射干涉仪,采用类迈克耳孙的光学结构,并结合低通小孔滤波,同时使用窗口傅里叶变换的方法解调单幅离轴载波条纹。与传统波前测量技术相比,所提出的准共光路的光学系统结构有效地抑制了系统像差及外部环境干扰等对测量结果的影响,实现高精度和高分辨率的波前探测。实验结果表明,该方法能够实现高精度的相位测量,且其重复精度达到了纳米量级。