An empirical model for the beams of radio pulsars

An empirical model for the beams of radio pulsars

Čájet eará veršuvnnaid (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...

Bibliográfalaš dieđut
Váldodahkkit:	Karastergiou, A, Johnston, S
Materiálatiipa:	Journal article
Giella:	English
Almmustuhtton:	2007

Geahča maid

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