Elongated beams, interpulses and the new millisecond pulsar

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1052

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DC Field	Value	Language
dc.contributor.author	Narayan, R.	-
dc.contributor.author	Radhakrishnan, V.	-
dc.date.accessioned	2006-01-03T04:32:16Z	-
dc.date.available	2006-01-03T04:32:16Z	-
dc.date.issued	1983-01-20	-
dc.identifier.citation	Current Science, 1983, Vol. 52, p46-49.	en
dc.identifier.issn	0011-3891	-
dc.identifier.uri	http://hdl.handle.net/2289/1052	-
dc.description.abstract	The prominent interpulse of the new millisecond pulsar is consistent with very short period pulsars having fan-like beams, as suggested earlier by an independent study. It is shown that all the available data on interpulse statistics support this picture, and also indicate that pulsars with perpendicular rotation and magnetic axes are absent at long periods.	en
dc.format.extent	256252 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.title	Elongated beams, interpulses and the new millisecond pulsar	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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