A Joint model for radio and gamma-ray emission from pulsars

Details A Joint model for radio and gamma-ray emission from pulsars A Joint model for radio and gamma-ray emission from pulsars

2003-03-11

arxiv.org/abs/astro-ph/0303231v1

Astronomy and Astrophysics

Astrophysics

5 pages, 2 figure, IAU Symposium No.214 on "High Energy Processes and Phenomena in Astrophysics", August, 2002, Suzhou, China,

Scientific paper

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.

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