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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2564

Title: Pulse fluctuation properties at 35 MHz
Authors: Asgekar, Ashish
Deshpande, A.A.
Issue Date: 2000
Publisher: Astronomical Society of the Pacific
Citation: ASP Conference Series, 2000, Vol.202, p161
Abstract: High time-resolution observations of pulsars were carried out at 35 MHz, using the Gauribidanur Radio Telescope (India), to study the spectra of intrinsic pulse-to-pulse fluctuations. Our sample consists of a few bright pulsars, each of which was observed for $\sim$1000~seconds so as to obtain long sequences of single-pulse data. The results, in terms of fluctuation features apparent at this radio frequency, are presented and compared with similar measurements at higher frequencies. We show that the picture of a circulating system of sub-beams emerges naturally from the behaviour apparent even at these long wavelengths.
Description: Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations). Pulsar Astronomy - 2000 and Beyond, ASP Conference Series, Vol. 202; Proceedings of the 177th Colloquium of the IAU held in Bonn, Germany, 30 August - 3 September 1999. (San Francisco: ASP). Eds. M. Kramer, N. Wex, and N. Wielebinski, p. 161
URI: http://hdl.handle.net/2289/2564
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?2000ASPC..202..161A
http://arxiv.org/abs/astro-ph/9911428
Copyright: 2000 Astronomical Society of the Pacific
Appears in Collections:Research Papers (A&A)

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