Radio pulsar emission altitudes

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DC Field	Value	Language
dc.contributor.author	Kapoor, R.C.	-
dc.contributor.author	Shukre, C.S.	-
dc.date.accessioned	2006-06-27T07:31:18Z	-
dc.date.available	2006-06-27T07:31:18Z	-
dc.date.issued	2002	-
dc.identifier.citation	Bulletin of the Astronomical Society of India, 2002, Vol.30, p695-696	en
dc.identifier.issn	0304-9523	-
dc.identifier.uri	http://hdl.handle.net/2289/1385	-
dc.description	Presented at the 21st meeting of the Astronomical Society of India, Pune, 2002.	en
dc.description.abstract	By attributing the often seen longitude offsets between the core and conal component centres of pulsar radio pulses to different emission altitudes, we present a new method for investigating these altitudes. Our method can explain these offsets and also sheds light on them.	en
dc.format.extent	52426 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The Astronomical Society of India	en
dc.rights	(2002) by the Astronomical Society of India.	en
dc.title	Radio pulsar emission altitudes	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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