机译：无线电极化梯度揭示星际气体中的低马赫数湍流
Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales 2006, Australia.;
ASTRON, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands. ,LeidenObservatory, Leiden University, PO Box 9513,2300 RA Leiden, The Netherlands. ,Department of Astrophysics/IMAPP, Radboud University Nijmegen, PO Box 9010,6500 GLNijmegen,The Netherlands.;
Astronomy Department, University of Wisconsin, Madison, 475 North Charter Street, Madison, Wisconsin 53711, USA.;
Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales 2006, Australia.,Australia Telescope National Facility, CSIRO Astronomy and Space Science, PO Box76, Epping, New South Wales 1710, Australia.;
Australia Telescope National Facility, CSIRO Astronomy and Space Science, PO Box76, Epping, New South Wales 1710, Australia.;
Australia Telescope National Facility, CSIRO Astronomy and Space Science, PO Box76, Epping, New South Wales 1710, Australia.;
Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales 2006, Australia.;
School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia;
Sydney Institute for Astronomy, School of Physics, The University of Sydney, New South Wales 2006, Australia;
机译：线性极化图梯度的星际湍流性质
机译：磁星际湍流对无线电同步加速器波动统计的影响
机译：磁星际湍流对无线电同步加速器波动统计的影响
机译：间隙湍流间歇性：弥漫性分子气体中的观察签名
机译：I.对140个紧凑型河外无线电源进行的22 GHz VLBI调查。二。在15 GHz和22 GHz的伽玛射线暴的VLBA极化观测。
机译：局部星际湍流的粉尘极化图
机译：无线电极化梯度揭示星际气体中的低马赫数湍流
