An empirical model for the beams of radio pulsars

An empirical model for the beams of radio pulsars

Pokaż inne wersje (1)

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...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy:	Karastergiou, A, Johnston, S
Format:	Journal article
Język:	English
Wydane:	2007

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