A Joint model for radio and gamma-ray emission from pulsars
Astrophysics
2007-05-23 v1
Abstract
Although pulsars can radiate electromagnetic wave from radio to gamma ray bands, we still have no a united model to understand the multi-band emission. In this paper the effort for a joint model is presented. The inverse Compton scattering (ICS) and a second acceleration process near the null charge surface are involved to account for the radio and the gama-ray emission, respectively. Various kind of pulse profiles and other observational properties can be reproduced.
Cite
@article{arxiv.astro-ph/0303231,
title = {A Joint model for radio and gamma-ray emission from pulsars},
author = {G. J. Qiao and K. J. Lee and H. G. Wang and R. X. Xu},
journal= {arXiv preprint arXiv:astro-ph/0303231},
year = {2007}
}
Comments
5 pages, 2 figure, IAU Symposium No.214 on "High Energy Processes and Phenomena in Astrophysics", August, 2002, Suzhou, China, in press