Linear Polarisation Properties of Pulsars at 35 & 327 MHz

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dc.creatorAsgekar, Ashish
dc.creatorDeshpande, A. A.
dc.date1999-11-23
dc.date.accessioned2026-07-07T02:34:37Z
dc.date.available2026-07-07T02:34:37Z
dc.descriptionWe 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.
dc.description2 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9911434
dc.identifierhttp://arxiv.org/abs/astro-ph/9911434
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15314
dc.subjectAstrophysics
dc.titleLinear Polarisation Properties of Pulsars at 35 & 327 MHz
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