Radio and gamma-ray emission from pulsars

Details Radio and gamma-ray emission from pulsars Radio and gamma-ray emission from pulsars

2003-03-11

arxiv.org/abs/astro-ph/0303232v1

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure, in the meeting on "Radio Pulsars", Crete 2002, in press

Scientific paper

The radiation of pulsars have been observed for many years. A few pulsars are discovered to have both radio and gamma-ray emission. Many models on pulsar radiation have been developed, but so far we are still lacking an elaborate model which can explain the emission from radio to gamma-rays in detail. In this paper we present a joint model for radio and gamma-ray emission, in which both the dominate emission mechanisms are inverse Compton scattering. The pulse profiles at radio and gamma-ray bands are reproduced for the Crab-like, Vela-like and Geminga-like pulsars, in good agreement with observations.

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