Phase-resolved Faraday rotation in pulsars
We have detected significant rotation measure (RM) variations for nine bright pulsars, as a function of pulse longitude. An additional sample of 10 pulsars showed a rather constant RM with phase, yet a small degree of RM fluctuation is visible in at least three of those cases. In all cases, we have...
Main Authors: | , , , , |
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Formato: | Journal article |
Idioma: | English |
Publicado em: |
2009
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