Please use this identifier to cite or link to this item:
http://hdl.handle.net/2289/4974| Title: | The topology and polarization of sub-beams associated with the `drifting' sub-pulse emission of pulsar B0943+10 - II. Analysis of Gauribidanur 35-MHz observations |
| Authors: | Asgekar, Ashish Deshpande, A.A. |
| Keywords: | radiation mechanisms non-thermal; pulsars general; pulsars individual: B0943+10 |
| Issue Date: | 2001 |
| Publisher: | Wiley Balckwell |
| Citation: | Monthly Notices of the Royal Astronomical Society, 2001, Vol.326, p1249 |
| Abstract: | In the previous paper of this series, Deshpande & Rankin reported results regarding the sub-pulse drift phenomenon in pulsar B0943+10 at 430 and 111MHz. This study has led to the identification of a stable system of sub-beams circulating around the magnetic axis of this star. Here, we present a single-pulse analysis of our observations of this pulsar at 35MHz. The fluctuation properties seen at this low frequency, as well as our independent estimates of the number of sub-beams required and their circulation time, agree remarkably well with the reported behaviour at higher frequencies. We use the `cartographic' transform mapping technique developed by Deshpande & Rankin in Paper I to study the emission pattern in the polar region of this pulsar. The significance of our results in the context of radio emission mechanisms is also discussed. |
| Description: | Restricted Access. |
| URI: | http://hdl.handle.net/2289/4974 |
| ISSN: | 0035-8711 1365-2966 (Online) |
| Alternative Location: | http://adsabs.harvard.edu/abs/2001MNRAS.326.1249A http://arxiv.org/abs/astro-ph/0110142 http://dx.doi.org/ 10.1111/j.1365-8711.2001.04664.x |
| Copyright: | 2001 Royal Astronomical Society |
| Appears in Collections: | Research Papers (A&A) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 2001_MNRAS_Vol.326_p1249.pdf Restricted Access | Restricted Access | 177.35 kB | Adobe PDF | View/Open Request a copy |
Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.