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...
| Autors principals: | , |
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| Format: | Journal article |
| Idioma: | English |
| Publicat: |
2007
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