Volume 418, Number 1, April IV 2004
|Page(s)||203 - 211|
|Section||Stellar structure and evolution|
|Published online||02 April 2004|
Properties of the linearly polarized radiation from PSR B0950+08
Astro Space Center, P. N. Lebedev Physical Institute, Leninskij Prospect 53, 117924 Moscow, Russia e-mail: firstname.lastname@example.org
Corresponding author: T. V. Shabanova, email@example.com
Accepted: 26 November 2003
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, , is about 3 times greater than the published value of (Taylor et al. [CITE]).
Key words: stars: neutron / stars: pulsars: general / stars: pulsars: individual: PSR B0950+08
© ESO, 2004
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