Pulsar "drifting" -subpulse polarization: No evidence for systematic polarization-angle rotations

R. Ramachandran, J. M. Rankin, B. W. Stappers, M. L A Kouwenhoven, A. G J Van Leeuwen

    Research output: Contribution to journalArticlepeer-review

    Abstract

    Polarization-angle density displays were given for pulsars B0809+74 and B2303+30, which exhibited no evidence of the systematic polarization-angle rotation within individual subpulses. The drifting subpulses of both pulsars exhibited linear and circular polarization which appeared to reflect the characteristics of two nearly orthogonally polarized emission modes. PSR B0809+74's subpulses appeared to exhibit the extraordinary PA rotation on the basis of early observation and analytical methods.
    Original languageEnglish
    Pages (from-to)993-999
    Number of pages6
    JournalAstronomy and Astrophysics
    Volume381
    Issue number3
    DOIs
    Publication statusPublished - Jan 2002

    Keywords

    • Polarisation
    • Radiation mechanisms: non-thermal
    • Stars: pulsars: B0809+74, B2303+30

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