Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-08-06
Astron.Astrophys.410:253-256,2003
Astronomy and Astrophysics
Astrophysics
4 pages. Accepted by A&A
Scientific paper
10.1051/0004-6361:20031190
The low-frequency profiles of some pulsars manifest temporal broadening due to scattering, usually accompanied by flat polarization position angle (PA) curves. Assuming that the scattering works on the 4 Stokes parameters in the same way, we have simulated the effect of scattering on polarization profiles and find that the scattering can indeed flatten the PA curves. Since the higher-frequency profiles suffer less from scattering, they are convolved with scattering models to fit the observed low-frequency profiles. The calculated flat PA curves exactly reproduce the corresponding observations.
Han Jian-Long
Li Xi-Han
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