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Radio pulsar emission altitudes

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.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.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.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

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