Properties of the linearly polarized radiation from PSR B0950+08

Details Properties of the linearly polarized radiation from PSR B0950+08 Properties of the linearly polarized radiation from PSR B0950+08

2004-02-24

arxiv.org/abs/astro-ph/0402558v2

Astron.Astrophys. 418 (2004) 203

Astronomy and Astrophysics

Astrophysics

18 pages, including 10 figures. Accepted for publication in A&A

Scientific paper

10.1051/0004-6361:20040058

Measurements of average pulse profiles made with a single linear polarization over the range 41-112 MHz are presented for PSR B0950+08. We show that the observed variable structure of the pulse profiles is a result of Faraday sinusoidal modulation of the pulse intensity with frequency. The rotation measure corresponding to this effect, RM = 4 rad/m^2, is about 3 times greater than the tabulated value of RM = 1.35 rad/m^2.

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