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Linear Polarisation Properties of Pulsars at 35 & 327 MHz

1999/11/23 by Ashish Asgekar, Asgekar, Ashish, A. A. Deshpande +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9911434

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

arxiv created 1999/11/23 · arxiv updated 2009/12/01

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.

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