Phenomenology of pulsar B0809+74's rotating subbeam system. II. "Carousel" configuration and polarization

Details Phenomenology of pulsar B0809+74's rotating subbeam system. II. "Carousel" configuration and polarization Phenomenology of pulsar B0809+74's rotating subbeam system. II. "Carousel" configuration and polarization

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...455..215r&link_type=abstract

Astronomy and Astrophysics, Volume 455, Issue 1, August III 2006, pp.215-221

Astronomy and Astrophysics

Astrophysics

3

Stars: Pulsars: Individual: B0809+74, Polarization, Radiation Mechanisms: Non-Thermal

Scientific paper

Building on results and analyses of previous works, the structure and polarization of B0809+74's subbeam "carousel" is delimited, but not fully solved. Some 8-10 subbeams are indicated for an equatorward sightline traverse and 25-40 for a polarward one. Either alternative indicates a subbeam circulation time much longer than predicted by theory. Polarized subbeam maps show complex structure and suggest that the star's polarized modes are angularly disjoint.

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