2003/03/11 by G. J. Qiao, K. J. Lee, Qiao, G. J. +5
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0303231
5 pages, 2 figure, IAU Symposium No.214 on "High Energy Processes and Phenomena in Astrophysics", August, 2002, Suzhou, China, in press
arxiv created 2003/03/11 · arxiv updated 2009/12/01
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.