An empirical model for the beams of radio pulsars

An empirical model for the beams of radio pulsars

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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...

書誌詳細
主要な著者:	Karastergiou, A, Johnston, S
フォーマット:	Journal article
言語:	English
出版事項:	2007

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