Observations of PSR 0950 + 08 at 103 MHz

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1567

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DC Field	Value	Language
dc.contributor.author	Deshpande, M. R	-
dc.contributor.author	Vats, Hari Om	-
dc.contributor.author	Janardhan, P	-
dc.contributor.author	Bobra, A. D	-
dc.date.accessioned	2007-05-10T05:45:36Z	-
dc.date.available	2007-05-10T05:45:36Z	-
dc.date.issued	1993	-
dc.identifier.citation	BASI, Vol. 21, pp. 613-614	en
dc.identifier.uri	http://hdl.handle.net/2248/1567	-
dc.description.abstract	n this article we report the possible cause of an enormously large enhancement (burst) in the ratio flux of PSR 0950 + 08. The burst was observed by two radio telescopes at Rajkot and Thaltej separated by 20 km. Simple folded data and cross correlogram brings out clearly the period of pulsar and indicate that the radio pulses remained intact in spite of their passage through the interplanetary medium. We argue that this burst is intrinsic to the source and not caused by the intervening medium.	en
dc.format.extent	159211 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Radio observations	en
dc.subject	Pulsar	en
dc.title	Observations of PSR 0950 + 08 at 103 MHz	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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