The geometry of PSR B0031-07
Astrophysics
2007-05-23 v1
Abstract
Here we present the results from an analysis of a multifrequency simultaneous observation of PSR B003107. We have constructed a geometrical model, based on an empirical relationship between height and frequency of emission, that reproduces many of the observed characteristics. The model suggests very low emission altitudes for this pulsar of only a few kilometers above the star's surface.
Keywords
Cite
@article{arxiv.astro-ph/0612684,
title = {The geometry of PSR B0031-07},
author = {R. Smits and D. Mitra and B. Stappers and J. Kuijpers and P. Weltevrede and A. Jessner and Y. Gupta},
journal= {arXiv preprint arXiv:astro-ph/0612684},
year = {2007}
}
Comments
Proceedings of the 363. WE-Heraeus Seminar on: Neutron Stars and Pulsars (Posters and contributed talks) Physikzentrum Bad Honnef, Germany, May.14-19, 2006, eds. W.Becker, H.H.Huang, MPE Report 291, pp.161-164