脉冲星在35与327 MHz的线偏振特性
天体物理学
2007-05-23 v1
摘要
我们报告了在35与327 MHz脉冲星辐射中线偏振的初步研究结果。为此我们利用了观测波段内差分法拉第旋转引起的光谱调制。我们通过与较高射电频率的现有测量结果进行比较，讨论了几个亮脉冲星的结果。
引用
@article{arxiv.astro-ph/9911434,
title = {Linear Polarisation Properties of Pulsars at 35 & 327 MHz},
author = {Ashish Asgekar and A. A. Deshpande},
journal= {arXiv preprint arXiv:astro-ph/9911434},
year = {2007}
}
备注
2 pages, 4 figures, To appear in the Proceedings of IAU Colloquium 177 : "Pulsar Astronomy - 2000 & Beyond", Ed. Kramer, Wex, & Wielebinski, ASP conf.Series. Gzipped PS file also available from http://www.rri.res.in/~ashish/html_files/reprints.html