arXiv · astro-ph/0402558
Properties of the linearly polarized radiation from PSR B0950+08
Abstract
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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T. V. Shabanova, Yu. P. Shitov. 2004-02-25. Properties of the linearly polarized radiation from PSR B0950+08. https://doi.org/10.1051/0004-6361%3A20040058
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