Pulse fluctuation properties at 35 MHz

Asgekar, Ashish; Deshpande, A.A.

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

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DC Field	Value	Language
dc.contributor.author	Asgekar, Ashish	-
dc.contributor.author	Deshpande, A.A.	-
dc.date.accessioned	2007-06-04T08:02:33Z	-
dc.date.available	2007-06-04T08:02:33Z	-
dc.date.issued	2000	-
dc.identifier.citation	ASP Conference Series, 2000, Vol.202, p161	en
dc.identifier.uri	http://hdl.handle.net/2289/2564	-
dc.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	en
dc.description.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.	en
dc.format.extent	193783 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of the Pacific	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2000ASPC..202..161A	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/9911428	en
dc.rights	2000 Astronomical Society of the Pacific	en
dc.title	Pulse fluctuation properties at 35 MHz	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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