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

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dc.creatorQiao, G. J.
dc.creatorLee, K. J.
dc.creatorWang, H. G.
dc.creatorXu, R. X.
dc.date2003-03-11
dc.date.accessioned2026-07-07T02:07:51Z
dc.date.available2026-07-07T02:07:51Z
dc.descriptionAlthough 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.
dc.description5 pages, 2 figure, IAU Symposium No.214 on "High Energy Processes and Phenomena in Astrophysics", August, 2002, Suzhou, China, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0303231
dc.identifierhttp://arxiv.org/abs/astro-ph/0303231
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5838
dc.subjectAstrophysics
dc.titleA Joint model for radio and gamma-ray emission from pulsars
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