Pulsar observations at 34.5 MHz using the Gauribidanur Telescope. I

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/758

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DC Field	Value	Language
dc.contributor.author	Deshpande, A.A.	-
dc.contributor.author	Radhakrishnan, V.	-
dc.date.accessioned	2005-12-19T11:06:34Z	-
dc.date.available	2005-12-19T11:06:34Z	-
dc.date.issued	1992	-
dc.identifier.citation	Journal of Astrophysics and Astronomy, 1992, Vol. 13, p151-165.	en
dc.identifier.issn	0250-6335	-
dc.identifier.uri	http://hdl.handle.net/2289/758	-
dc.description.abstract	This paper reports measurements of pulse profiles at 34.5 MHz of eight pulsars using the Gauribidanur Radio Telescope. None of the eight pulsars show any significant interpulse emission at this frequency, which conflicts with an earlier claim from 25 MHz observations. With the exception of one pulsar (PSR 0943 + 10), all the observed pulsars show turnovers at frequencies above 35 MHz in their spectra. Also reported are attempts to study the short and long term variations in the pulsar signals at this low frequency.	en
dc.format.extent	1336155 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences, Bangalore, India.	en
dc.rights	Indian Academy of Sciences, Bangalore, India.	en
dc.subject	pulsars;	en
dc.subject	interstellar scattering;	en
dc.subject	dispersion;	en
dc.title	Pulsar observations at 34.5 MHz using the Gauribidanur Telescope. I	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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