| Issue |
A&A
Volume 405, Number 3, July III 2003
|
|
|---|---|---|
| Page(s) | 795 - 801 | |
| Section | Astrophysical processes | |
| DOI | https://doi.org/10.1051/0004-6361:20030699 | |
| Published online | 30 June 2003 | |
On the search for coherent radiation from radio pulsars
1
Department of Astrophysics, University of Nijmegen, The Netherlands
2
Stichting “Astron”, PO Box 2, 7990 AA Dwingeloo, The Netherlands
3
Astronomical Institute “Anton Pannekoek”, Amsterdam, The Netherlands
4
Kapteyn Institute, University of Groningen, Groningen, The Netherlands
Corresponding author: J. M. Smits, roysm@astro.kun.nl
Received:
10
February
2003
Accepted:
6
May
2003
We have examined data from pulsars B0950+08 and B0329+54 for evidence of temporally coherent radiation using the modified coherence function (MCF) technique of Jenet et al. (2001). We consider the influence of both instrumental bandpass and interstellar propagation effects. Even after removal of the effects due to the instrumental bandpass, we detect a signature in the MCF of our PSR B0329+54 data which is consistent with the definition of a coherent signal. However, we model the effects due to interstellar scintillation for this pulsar and show that it reproduces the observed signature. In particular, the temporal coherence time is close to the reciprocal of the decorrelation bandwidth due to diffractive scintillation. Furthermore, comparison of the coherence times of three pulsars reported by Jenet et al. (2001) with their expected diffractive decorrelation bandwidths suggests that the detection of coherence in these pulsars is also likely a result of interstellar scintillation, and is not intrinsic to the pulsars.
Key words: radiation mechanisms: general / stars: neutron / pulsars: general / pulsars: individual: B0329+54, B0950+08
© ESO, 2003
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