An empirical model for the beams of radio pulsars

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...

תיאור מלא

מידע ביבליוגרפי
Main Authors: Karastergiou, A, Johnston, S
פורמט: Journal article
שפה:English
יצא לאור: 2007
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