Linear Polarisation Properties of Pulsars at 35 & 327 MHz
Astrophysics
2007-05-23 v1
Abstract
We report preliminary results of our study of linear polarization in the pulsar emission at 35 & 327 MHz. We have exploited for this purpose the spectral modulation resulting from the differential Faraday rotation across the observed band. We discuss the results on a few bright pulsars by comparing them with the existing measurements at higher radio frequencies.
Cite
@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}
}
Comments
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