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The GeV to TeV view of SNR IC443: predictions for Fermi

AutorRodríguez, Ana Yaiza; Torres, Diego F. ; Cea del Pozo, Elsa de
Palabras claveSNR (individual IC 443)
γ-rays: observations
γ-rays: theory
[PACS] Supernova remnants
[PACS] X- and γ-ray telescopes and instrumentation
Fecha de publicación17-ene-2009
CitaciónProceedings of the 6th Workshop on Science with the New Generation of High Energy Gamma-Ray Experiments (SciNeGHE '08)
ResumenWe present a theoretical model that explains the high energy phenomenology of the neighborhood of SNR IC 443, as observed with the Major Atmospheric Gamma Imaging Cherenkov (MAGIC) telescope and the Energetic Gamma-Ray Experiment Telescope (EGRET). We also discuss how the model can be tested with observations by the Fermi Gamma-ray Large Area Space Telescope. We interpret MAGIC J0616+225 as delayed TeV emission of cosmic-rays diffusing from IC 443 and interacting with a known cloud located at a distance of about 20 pc in the foreground of the remnant. This scenario naturally explains the displacement between EGRET and MAGIC sources, their fluxes, and their spectra. Finally, we predict how this context can be observed by Fermi.
Descripción9 pages, 4 figures.-- PACS: 98.38.Mz, 95.55.Ka.-- Contributed to: 6th Workshop on Science with the New Generation of High Energy Gamma-Ray Experiments (SciNeGHE '08), Padova, Oct 2008.-- Original presentation available.
Versión del editorhttp://arxiv.org/abs/0901.2615
Aparece en las colecciones: (ICE) Comunicaciones congresos
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