Radio Polarization and Geometry of PSR J1119-6127

Details Radio Polarization and Geometry of PSR J1119-6127 Radio Polarization and Geometry of PSR J1119-6127

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...20111804c&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #118.04; Bulletin of the American Astronomical Society, Vol. 34, p.1298

Other

Scientific paper

Using 1400-MHz archival data from the Parkes radio telescope, we present radio polarization characteristics for PSR J1119-6127, a very young pulsar notable for its large magnetic field. We compare the polarization features of PSR J1119-6127 with those of other young pulsars (e.g., PSR J1513-5908) and discuss the pulsar in the context of a recent theoretical model of pulsar spin-down; this spin-down model can in principle be tested with polarization and timing data from this pulsar. Constraints on the pulsar's emission geometry obtained from a rotating vector model fit to the available position angle data are not sufficient to test the spin-down model, but additional data may allow a significant test in the future.

Affiliated with

Also associated with

No associations

Rating

Radio Polarization and Geometry of PSR J1119-6127 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radio Polarization and Geometry of PSR J1119-6127, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio Polarization and Geometry of PSR J1119-6127 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1891194