| Issue |
A&A
Volume 418, Number 1, April IV 2004
|
|
|---|---|---|
| Page(s) | 203 - 211 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20040058 | |
| 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: shitov@prao.psn.ru
Corresponding author: T. V. Shabanova, tvsh@prao.psn.ru
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. [CITE]).
Key words: stars: neutron / stars: pulsars: general / stars: pulsars: individual: PSR B0950+08
© ESO, 2004
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