An empirical model for the beams of radio pulsars

An empirical model for the beams of radio pulsars

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Motivated by recent results on the location of the radio emission in pulsar magnetospheres, we have developed a model which can account for the large diversity found in the average profile shapes of pulsars. At the centre of our model lies the idea that radio emission at a particular frequency arise...

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Bibliografiske detaljer
Main Authors:	Karastergiou, A, Johnston, S
Format:	Journal article
Sprog:	English
Udgivet:	2007

Lignende værker

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High frequency observations of southern pulsars
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Multi-frequency integrated profiles of pulsars
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New pulsar rotation measures and the Galactic magnetic field
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Absolute polarization position angle profiles of southern pulsars at 1.4 and 3.1 GHz
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Simultaneous single-pulse observations of radio pulsars V. On the broadband nature of the pulse nulling phenomenon in PSR B1133+16
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The variability of radio pulsars
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