A&A 418, 203-211 (2004)
Properties of the linearly polarized radiation from PSR B0950+08T. V. Shabanova and Yu. P. Shitov
Astro Space Center, P. N. Lebedev Physical Institute, Leninskij Prospect 53, 117924 Moscow, Russia
(Received 30 July 2002 / 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. 1993).
Key words: stars: neutron -- stars: pulsars: general -- stars: pulsars: individual: PSR B0950+08
Offprint request: T. V. Shabanova, email@example.com
© ESO 2004