Radio Polarization and Spectra of Variable Extragalactic Objects

该项目的目标是研究活动星系核和类星体射电发射区的物理条件，以便了解高能等离子体在具有时变通量和偏振的天体中的产生和流动。主要数据来自密歇根大学26米射电望远镜进行的长期监测项目。对这些数据进行建模，以确定活动星系核的射电发射区的性质和动力学。***

ABSTRACT AST-9421979 Aller, Hugh The goal of this project is to investigate the physical conditions in the radio emitting regions of active galactic nuclei and quasars in order to understand the generation and flow of high energy plasma in objects exhibiting time-variable flux and polarization. The primary data are from a long term monitoring program conducted with a U. of Michigan 26-meter radio telescope. The data are modeled to determine the properties and dynamics in the radio-emitting regions of active galactic nuclei. ***