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...
| Principais autores: | , |
|---|---|
| Formato: | Journal article |
| Idioma: | English |
| Publicado em: |
2007
|