Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1385
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dc.contributor.authorKapoor, R.C.-
dc.contributor.authorShukre, C.S.-
dc.date.accessioned2006-06-27T07:31:18Z-
dc.date.available2006-06-27T07:31:18Z-
dc.date.issued2002-
dc.identifier.citationBulletin of the Astronomical Society of India, 2002, Vol.30, p695-696en
dc.identifier.issn0304-9523-
dc.identifier.urihttp://hdl.handle.net/2289/1385-
dc.descriptionPresented at the 21st meeting of the Astronomical Society of India, Pune, 2002.en
dc.description.abstractBy 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.extent52426 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe Astronomical Society of Indiaen
dc.rights(2002) by the Astronomical Society of India.en
dc.titleRadio pulsar emission altitudesen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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